198lApJS ... 45. .259W © 1981.TheAmericanAstronomicalSociety.Allrightsreserved.PrintedinU.S.A. The AstrophysicalJournalSupplementSeries,45:259-334,1981February by Strömberg(1925),Moore(1932),Edmondson(1935), be trulycomprehensiveinits treatmentofallavailable most recently,HarrisandRacine(1979).Whileeachof Mayall (1946),Kinman(1959),Kukarkin(1974),and, of Kinman,whichisstillin widespread use,isthelastto years sincethosestudies,severalotherradialvelocity these compilationsincorporatesintermediateresults,that Zinn (1974),andHartwickSargent(1978)arealso obtained velocitiesof18clusters.Inthemorethan60 first obtainedinthepioneeringsurveysbySlipher(1918, individual starsforclosestudyhasbeengreatlyex- individual clustershavebeenpublished,ofwhichthose noteworthy fortheirextent.Atthiswriting,anambi- (1959). ThesurveysofJoy(1949),vandenBergh(1969), ford (1918,1919a,6),atMountWilson,whotogether panded inthepastdecadethroughuseofimage-tube both theirextentandaccuracy.Theaccessibilityof NGC 5139(coCen)byHarding(1965),and5272 radial velocityinterferometer,whichpromisesasubstan- Hesser andShawlisunderway,usingaFabry-Perot sive, byfar,arethoseMayall(1946)andKinman surveys havebeenpublished,ofwhichthemostexten- 78-12309. (M 3)byGunnandGriffin(1979)arenoteworthyfor of NGC104(47Tue)byFeastandThackeray(1960), (see Smith,Hesser,andShawl1976;Hesser tial improvementinthedataavailableformanyclusters correlation techniques. spectra, photoelectricradialvelocityspectrometers,and tious redeterminationofglobularclustervelocitiesby 1919, 1922,1924),atLowellObservatory,andbySan- 1977). Inaddition,anumberofdetailedstudies 1 Compilations ofclustervelocitieshavebeenpublished Radial velocitiesofgalacticglobularclusterswere SupportedinpartbyNationalScience FoundationgrantAST © American Astronomical Society •Provided by theNASA Astrophysics DataSystem velocities in4dwarfspheroidalsatellitesoftheGalaxy.Weightedmeanforeach89 Subject headings:clusters:globular—stars:catalogs systems inthecatalogandAppendixarecalculated. and 85globularclustersarepresentedinthebodyofcatalog;anAppendixlistspublishedradial to 1980isassembledhere.Knownsystematicerrorsinthedataarediscussed,andon686stars A catalogofallstellarandintegratedradialvelocitiesgalacticglobularclusterspublishedprior 1 A CATALOGOFRADIALVELOCITIESINGALACTICGLOBULARCLUSTERS I. INTRODUCTION Department ofAstronomy,UniversityIllinoisatUrbana-Champaign Received 1980February25;acceptedJuly9 R. F.Webbink ABSTRACT 259 log oftheclusterexists,those starsidentifiedinthat catalog areUstedfirstinnumerical order,foUowedby ual starswithinthecluster.Whereanastrometriccata- originally intheNewGeneralCatalogue(Dreyer1888) and thusplacestheNGCclustersinnumericalorder. spectra areUstedfirst,followedbyvelocitiesforindivid- For eachcluster,radialvelocitiesbasedonintegrated ascension atequinox1860.0.Thisistheadopted with typicaluncertaintiesoflessthan0Tineachcoordi- pendix, alongwiththeirequatorialandgalacticcoordi- January 1areincludedhere.Tableliststhe85globular ment oftheclustervelocitiesonthisbasis.Tobest comprehensive listingofallavailableglobularcluster data. Nocatalogofindividualstellarandclusterveloci- nates. Thesecoordinateshavebeencompiledfrom radial velocitydataandtoprovideasystematicreassess- ties existsassuch. weighting individualvelocitiesandthecalculationof published radialvelocities,and§IVwiththemethodof nate. numerous sourcesandrefertothedynamicalcenters, satellites oftheGalaxywhichareincludedinAp- clusters includedinthecatalog,plus4dwarfspheroidal the author’sknowledge,alldatapublishedpriorto1980 and thefourdwarfspheroidalsystemsinAppendix ties foreachofthe85globularclustersincatalog stellar andclustermeanvelocities.Thededucedveloci- Section IIIdealswithsystematiccorrectionstothe are tabulatedin§V. catalog. Inmanycases,no astrometric catalogexists;a finaUy anyvariablestarsnot includedintheprimary any nonvariablestarsidentified inothersources,and The presentcatalogisintendedtofilltheneedfora Ousters arearrangedinorderofincreasingright The formatofthecatalogisdescribedindetail§II. II. DESCRIPTIONOFTHECATALOG 198lApJS ... 45. .259W NGC 288 NGC 1261 NGC 364 NGC 104(47Tue) NGC 1851 Pal 1 NGC 2298 NGC 1904(M79) Pal 2 Eridanus (GC10422-213) NGC 2808 NGC 2419 Cluster NGC 3201 Pal 3(SextansC) NGC 4590(M68) NGC 4372 NGC 4147 Pal 4(UrsaMajor) NGC 5024(M53) NGC 4833 NGC 5286 NGC 5139(o)Cen) NGC 5466 NGC 5272(M3) NGC 5634 NGC 5904(M5) NGC 5824 NGC 5694 NGC 5986 NGC 5927 NGC 6121(M4) NGC 6093(M80) Pal 14(A-vdB) NGC 6171(M107) NGC 6139 NGC 6205(M13) NGC 6254(M10) NGC 6218(M12) NGC 6362 NGC 6293 NGC 6284 NGC 6273(M19) NGC 6266(M62) NGC 6229 NGC 6397 NGC 6388 NGC 6356 NGC 6341(M92) NGC 6333(M9) NGC 6304 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Clusters IncludedintheCatalog 00 2153 00 5019 03 2601 03 1054 01 32 04 4255 04 2235 05 1228 06 4713 09 1105 07 3446 05 2208 11 2637 10 1534 10 0258 12 2253 12 0733 13 2347 13 1028 14 2700 12 3648 13 3953 12 5614 13 4316 14 03 15 0054 14 3642 15 4247 15 2423 15 1601 16 1403 16 2943 16 2417 16 2031 16 0841 16 4534 17 16 17 0703 16 5431 16 4438 16 3953 17 3637 17 3238 17 1535 17 1122 17 0125 16 5933 16 5802 17 2040 17 2645 a (1950) h ms TABLE 1 260 +31 17.5 +79 24.7 -72 21.5 -55 24.1 -71 07.0 -21 18.0 -26 51.1 +38 59.7 +29 15.3 +00 19.0 -40 06.1 +18 49.2 -35 56.7 -24 34.2 -64 39.4 +28 37.8 +18 26.0 -46 09.8 -26 28.1 -72 22.6 +28 46.5 -70 36.4 -47 13.1 +02 15.8 -51 07.5 +15 05.2 -26 19.4 -05 45.3 -37 37.4 -32 52.4 -50 30.0 -26 24.5 -22 51.2 -12 56.9 -38 44.3 -K7 36.9 +36 33.2 +43 11.4 -24 41.8 -26 11.8 -30 02.4 -04 01.6 -01 51.6 -26 31.2 -44 42.3 -67 00.7 -18 27.9 -53 39.0 -17 46.1 -29 24.4 6 (1950) 305.895 301.534 151.193 270.537 218.105 227.231 244.512 130.065 245.626 282.193 170.532 202.293 277.231 240.142 180.370 299.625 300.997 252.847 332.960 303.606 042.220 309.101 042.156 003.859 342.210 311.615 331.056 028.744 326.604 332.555 337.029 350.975 352.673 003.372 342.365 355.825 345.556 357.620 358.347 356.870 353.575 015.136 073.638 015.715 059.006 338.163 325.554 068.339 005.544 006.723 +19.029 -89.378 -44.989 -52.125 -46.247 +41.867 +25.243 -35.036 -09.069 -41.332 +71.801 +08.640 +77.189 +36.052 -16.006 -29.350 +79.764 -11.252 -09.878 +10.568 +78.708 +14.971 -08.015 +73.585 +30.360 +49.260 +46.797 +22.070 +42.197 +13.274 +04.860 +15.974 +23.013 +06.939 +19.463 +05.374 +40.306 +10.220 +09.939 +09.382 +07.318 +23.073 +34.858 +10.705 +07.834 +26.313 +40.915 -06.738 -11.959 -17.570 198lApJS ... 45. .259W Cluster NGC 6440 NGC 6402(M14) NGC 6441 NGC 6544 NGC 6528 NGC 6522 NGC 6553 NGC 6541 NGC 6624 NGC 6584 NGC 6637(M69) NGC 6626(M28) NGC 6652 NGC 6642 NGC 6638 NGC 6656(M22) NGC 6715(M54) NGC 6681(M70) NGC 6723 NGC 6712 NGC 6779(M56) NGC 6752 NGC 6838(M71) NGC 6809(M55) Pal 11 NGC 6934 NGC 6864(M75) NGC 7078(M15) NGC 7006 NGC 6981(M72) NGC 7099(M30) NGC 7089(M2) Ursa Minor(DDO199) NGC 7492 Draco (DDO208) Pal 13(Pegasus) Pal 12(Capricorn) Fornax Sculptor © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Dwarf SpheroidalSystems a (1950) 18 0023 17 4649 17 4555 17 3458 18 0137 18 1438 18 0611 18 0415 18 0425 18 2808 18 2128 18 2028 18 2852 18 2751 18 51 18 3957 18 3321 18 3229 19 0628 18 5020 19 3649 19 1439 18 5611 19 5131 19 4232 TABLE 1—Continued 21 2733 20 5043 20 3145 20 0308 17 1913 15 0812 23 0550 23 0414 21 4350 21 3732 21 3053 20 5909 02 3750 00 5744 h ms 261 <$ (1950) +30 05.6 -37 02.3 -20 20.7 +18 38.7 -25 00.3 -43 43.4 -30 03.6 -30 02.2 -03 13.1 -25 32.0 -30 23.3 -52 14.2 -25 55.1 -33 02.0 -32 23.1 -24 53.8 -31 04.5 -60 03.9 -30 32.7 -08 46.2 -23 56.9 -23 30.7 -36 42.1 -32 20.5 -08 07.7 +15 59.4 +07 14.0 +11 56.8 +12 30.2 +57 57.5 +67 23.0 -23 24.4 -01 02.8 -12 43.6 -22 03.9 -34 44.4 -34 00.4 -15 52.8 -21 29.1 353.532 349.286 342.143 005.837 001.138 001.026 007.729 021.323 001.722 002.788 005.253 025.352 009.814 007.896 007.799 336.495 005.607 002.853 009.890 001.533 000.070 062.659 056.740 031.806 008.798 104.969 237.294 287.685 020.304 053.395 087.104 027.179 053.371 065.013 063.769 035.163 052.104 030.509 086.363 +03.800 +14.805 +08.336 -11.188 -03.929 -05.006 -10.270 -03.029 -02.201 -12.509 -07.152 -05.580 -07.913 -04.175 -25.628 -07.552 -11.378 -06.439 -16.415 -23.268 -17.299 -14.087 -04.318 -04.560 -15.576 +44.843 +34.746 -46.835 -27.313 -19.407 -32.683 -63.480 -42.698 -18.894 -25.748 -65.654 -47.681 -35.770 -83.133 198lApJS ... 45. .259W 262 identifications foreachclusterisintendedtoguard adopted asaprimaryreferenceforstellaridentifica- suitable photometricsurveyoftheclusterwasthen against multipleentriesforstarswhichareinfactidenti- tions. Theuseofasingleprimarysourcestellar cally thesame,althoughidentifieddifferentlyindiffer- lowed, inturn,byindividualstarsidentifiedaprimary instances, meanvelocitiesforseveralstarsnotindividu- ent sources. number ofstarsincludedinthemean.Theyarefol- columns: by Sandage[Sg]).Referencestarsinthepropermotion cluster, secondandthirdreferencesaredistinguishedby by aletterprefixforwhichreferenceisprovidedatthe spectra inthetableandareidentifiedmerelyby ally identifiedwerepublished.Thesefollowintegrated bers inparentheses(e.g.,Ga(32)=K188NGC6205). one referencebythesameauthorsappearsinasingle source, asindicatedabove.Thissourceisitselfidentified velocities. Wheremorethanonemeasurementhasbeen mally thisistheidentificationgivenstarin necessary. Theyare: repeated identificationinthetablewasdeemedun- the samearticlefordifferentclusters;wheremorethan throughout thecatalog,butthesedonotalwaysreferto or combinationsofauthors,areassignedthesameprefix end ofthetabulationforeachcluster.Individualauthors, spectra aredesignated“Int”inthiscolumn.Inafew phase forvariablestarsofknown periods. in chronologicalorderor orderofmeanphotometric lished values,whichfollow. Publishedvaluesarelisted published foragivenstar,the firstentryistheweighted a numberintheprefix(e.g.,Sglreferstosecondpaper mean stellarvelocitydeduced fromtheindividualpub- from theoneincolumn(1). from hisclusterstarsbyenclosingreferencestarnum- study byGamalej(1948)havebeendistinguishedhere as notedinthefollowingcolumn,theseareheliocentric source foritsradialvelocity,ifthatidentificationdiffers CPD—Cape PhotographicDurchmusterung CoD—Cordoba Durchmusterung -1 HD—Henry DraperCatalogue HV—Harvard VariableStar BD—Bonner Durchmusterung The datatabulatedinthecatalogarearranged14 Variable stardesignationsintheGeneralCatalogueof A fewabbreviationsareinsuchwidespreadusethat 2) AltID.—Alternativestellaridentification.Nor- 3) v.—Publishedradialvelocity(inkms')Except 1) PrimaryID,—Stellaridentification.Integrated r © American Astronomical Society •Provided by theNASA Astrophysics DataSystem V—Third CatalogueofVariableStarsinGlobular Clusters (Hogg1973). 1969), anditssupplements. Variable Stars,3rdedition(Kukarkinetal, WEBBINK -1 letter oracombinationofletters: Where azero-pointcorrectiontovisindicated,the below. must beappliedtothevelocityincolumn(3)obtain Derivation ofthesesystematiccorrectionsisdiscussed ture ofthiscorrectionisindicatedbyasuffixone an absoluteheliocentricstellarradialvelocity.Thena- where probableerrorsarequotedbythesource, was followedbyestimatingtheerrorfromreciprocal nal errorprovedimpossible,MayalTs(1946)procedure tion. Ingeneral,publishederrorestimateshavebeen standard errorincludestheofcorrec- dispersion ofthespectrogram: estimate wasformedwherepossiblefromtheinternal When noestimateoftheerrorhasbeenpublished,an adopted withoutalteration(exceptforzero-pointerrors); agreements ofthevelocitiesgiveninthatsource. standard errorwascomputedusingtheformula here. in ÀmmatHy.Forintegratedspectra,ewasin- (for stellarspectra),whereAisthereciprocaldispersion represents theerrorin stellar velocity.Thisdistinc- constituent velocities(see § IVbelow)andtherefore mean computedfromthe internal agreementofthe weighted meanvelocities,eisthestandarderrorof give adequateestimatesoftheerrorstypicalimage- creased byafactorof1.5.Thisprescriptionappearsto the errorofanindividualobservation.However,for tube spectra,butgoodqualitydirectphotographicspec- tion isimportantforvariable stars. tra areprobablysomewhatmoreaccuratethanreflected r -1 _1 p—correction ofaperiodicradial-velocityvariable h—correction fromgeocentrictoheliocentricradial 4) At>.—Asystematiccorrection(inkms)which a—correction toanemission-linevelocityforitssys- z—zenith correction,presumablyduetothedisplace- As alastresort,wheredirectassessmentoftheinter- 5) e.—Estimatedstandarderrorinv(inkms). r—zero-point correction,arisingfromthechoice 6) Ref.—Sourceofthepublished radialvelocity. In thecasesofindividualstellarvelocities,erepresents r velocity; image ofastaronthespectrographslit,arising reference standard; (whether deliberateoraccidental)ofamoving ment ofthephotographicimagefromvisual for phase; spectrum; tematic offsetwithrespecttotheabsorption-line from differentialatmosphericrefraction. /2-1 6=0.96^ kms(2) Vol. 45 198lApJS ... 45. .259W velocity appearattheleft-handsideofthiscolumn; velocity. Weightsofvelocitiescombinedinthestellar photometry iscited,wheneveravailable,followedby included inthiscatalog,althoughsearchwasnot photoelectric photometryinthesamecolors,photo- most extensiveandreliableisgivenhere,ratherthan completely exhaustive.Foragoodmanystars,photome- have beenpublished;theauthorhaslistedmore below inthesectiondescribingcalculationofstellar No. 2,1981 ple lineartransformationsduetoArp(1955a,b): ence. Whereachoiceexistsbetweenphotographicand forming meansofthepublishedmaterial.Three-color authors. Thatwhichwas(somewhatarbitrarily)judged search wasmadeforbroadbandphotometryofthestars based ontheindividualspectraaregivenwhereverpos- hydrogen lines.Insomecases,twoormoreassignments cluster mean,adashappearsinthiscolumn.Calculation has beenrejectedfromcalculationofthestellaror surement incomputingthestellarvelocityorcluster have beenpublishedbyvariousauthorsforafewclus- color photometryinthe(m,m)or(P,V)system electric photometryhas,ofcourse,beenselected.In mum isgiven. reliable oraccurateonesinhisopinion,butthischoiceis classifications basedonthesamespectrogramsusing of theseweightsandrejectioncriteriaarediscussed those combinedincomputingtheclustervelocityappear of thephotometry,employingthroughoutsim- exists. Althoughmoresopmsticatedtransformations some casesUBVphotometrydoesnotexist,buttwo- two-color orsingle-colorphotometryinorderofprefer- try intheJohnsonUBVsystemisavailablefromseveral able. Thesefrequentlydiffersignificantlyfromspectral tions, basedonmetalliclines,aregivenwhereavail- and clustervelocities. at theright-handsideofcolumn.Whereavelocity indicated, whereveravailable. Inafewinstances,iso- sible. Foreclipsingbinaries,thespectraltypeatmaxi- frequently arbitrary.Forvariablestars,spectraltypes lated measurementsintheUBV systematasinglephase ters, wehavepreferredheretocitetheoriginalsources magnitude. Forthethreeeclipsing binariesincludedin For variablestars,mean magnitudes andcolorsare are available;thesedenoted byavfollowingtheV FVpg 7) Wt.—Weightassignedtothisradialvelocitymea- 9) Ref.—Sourceofthespectraltype. 8) Sp.—Spectraltype.FullMKspectralclassifica- 10) V.—JohnsonV(visual)magnitude.Anextensive © American Astronomical Society •Provided by theNASA Astrophysics DataSystem B— F=0.91(P—F)+0.18.(5) B-V=0M{m-m)+021, (4) pgpv V=m, (3) pv RADIAL VELOCITIESINGLOBULARCLUSTERS were encountered.Thesedifferenceshavebeennotedin variable starsofknownphotometricperiodand vidual observations,membershipofstarsrejectedin given. ferences betweenphotometryfromtwo(ormore)sources the catalog,magnitudeandcolorsatmaximumare velocity orthatcitedforthephotometry. but theyarenotincludedamongthesepropermotion proper motionsurveysinresolvingquestionsofcluster period (inthecaseofveryshortpulsators), binaries andsomelonger-periodRVTaurivariables. epoch ofobservation,themeanphotometricphase,, computing theclustervelocity,andadditionalidentifica- relevant informationregardingtheparticularsofindi- columns (10)-(12). the remarks,butnoefforthasbeenmadetoresolve bers, adiscussionofthemembershipproblemcanusu- have beenrejectedasfieldstarsordoubtfulmembers, proper motionfieldstarsnearNGC6397.Where Where theplatesfromwhichvelocitieshavebeende- variables buttoprimaryminimumfortheechpsing corresponding toHghtmaximumformostpulsating of thiscolumn.Exceptasnoted,thesearecomputed the starorobservation.Thiscolumnanditscontinua- them. (1976/?). Inaddition,Cannon(1974)identifiesseveral 6838, Sanders(1971);andforNGC7078,Cudworth (1979a); forNGC6341,Cudworth(1976c); 6205, CudworthandMonet(1979) (1979Z>); forNGC5904,Cudworth(1979c); membership inseveralwell-studiedclusters:forNGC rived coverasignificantfractionofthephotometric tions beyondthoselistedincolumns(1)and(2).For tion attheendofeachclusterlistingcontainadditional ally befoundineitherthesourcecitedforradial 5139, Woolley(1966);forNGC5272,Cudworth from theephemeridesUstedbyHogg(1973),with<£>=0 the observedradialvelocityislistedatleft-handside surveys ortheyarenotobviousradial-velocitynonmem- the durationofexposureinphaseisindicated. periodic, anditsphasedependence canbeestablished, variables aswell.Wherethis radialvelocityvariationis A fewinstancesofclearsystematiczero-pointdif- Considerable usehasbeenmadeofthefollowing 13) Ref.—SourceoftheUBVphotometrycitedin 14) Remarks.—Additionalinformationpertainingto 12) Î/-Æ.—(seecol.[10]). 11) B—V.—(seecol.[10]). Photometric variablesare, as arule,radialvelocity III. SYSTEMATICCORRECTIONS i) PhaseCorrections(p) a) VariableStars 263 198lApJS ... 45. .259W pressed. Ontheotherhand,itisdifficulttoweight wide excursionsoftheradialvelocityduringphases italics arethosewhoseinclusionisnotsignificantatthe where isagainthephotometricphase(0<<¡><1).The where fewornoobservationsexistcaneasilybesup- many respectsaneye-interpolationproducesthemost uted veryunevenlyinphotometricphase,definitionof NGC 6779)nosignificantperiodiccomponentstothe in Figures\a-1j.Foranotherfivevariables(V19NGC which yieldedstatisticaDysignificantresults.Termsin were madetoFourierfittheradialvelocitydataofeach corrections quotedinthecatalogarecomputedfrom y-velocity is,ofcourse,givenbythevaluea,andits confidence levelasdeterminedbyastandardF-test.The obtain aradialvelocitycurveobjectivelyfromdataof or itsy-velocity. observations objectivelyinsuchaprocedure,ortode- termined bydirectintegrationofradialvelocitycurve. the y-velocityofabsorption-linesystemcanbede- more thanhalfthephotometricperiod.Thecomponents periodic variablewith{a)sufficientnumbersofobserva- remaining termsintheFourierseriesfittodata. formal uncertaintycanbereadilycomputed.Thephase gives nosignificantimprovementinthefit,ata75% series istruncatedwhentheinclusionoffurtherterms a weightedleast-squaresfittothedata, as aFourierseriesofvelocitycomponents,obtainedby fine quantitativelytheuncertaintyinresultantcurve aesthetically satisfyingrepresentationofthecurve,since published values,whichwere basedessentiallyonan in largevariationsthe interpolated radialvelocity radial velocitieswerefound. 90% confidencelevel.Thefitstothedataareillustrated assorted weightsandphasesistorepresentsuchacurve the radialvelocitycurvepresentsaseriousproblem.In 264 ity isinfactoutstanding agreementwithpreviously relatively poorphasecoveragenearæ0.8hasresulted large numberofFourierterms(andhenceabody obvious. Theyarewell-illustratedbythecurveobtained 5466, VI1NGC6205,VI6218,andV3V6 thus obtainedarelistedinTable2,forthosevariables tions topermitsuchaprocedureand{b)coverageover curve. Nevertheless,theincluded termsaresignificantat for V42NGC5904.Thisvariableevidentlypossessesa of radialvelocitydata)foradequaterepresentation.The saw-tooth-type radicalvelocitycurve,whichrequiresa a highconfidencelevel,and thededucedsystemicveloc- 0 The procedureadoptedherewhichdoes,inprinciple, Since radialvelocitymeasurementstendtobedistrib- The pitfallsinthefittingprocedureusedhereare Variables withwell-definedvelocitycurves.—Attempts © American Astronomical Society •Provided by theNASA Astrophysics DataSystem v=a+ 2(anCOs27rn+bsm27rn),(6) r0n n=\ N WEBBINK 3/21 virial argumentsufficestorelatethemeanstellarradius, velocity forV65NGC3201wasobtainedatornear period, andinclinationofthebinary.Theseproperties whose amplitudedependsonthemass,massratio,orbital where Misthestellarmass. Thus,wefind proportional tothelogarithmicamplitudeofvari- has beenfollowed.Wesupposethatthelogarithmic inclination /æ90°. period (Hogg1973),anddurationofprimaryeclipse phase correctionis,inthiscase,estimatedontheas- (1973). Thisephemerisneedsconfirmation,asaconsid- (Tiller 1978),accordingtotheephemerisgivenbyHogg 6838 wasobtainedshortlybeforeprimaryminimum color andlightcurveofthevariable.Infact,sole may beestimatedbyjudiciousinterpretationofthe The radialvelocitycurveisthusasimplesinecurve, of proportionalitybeingjust thepulsationconstantß), R, tothepulsationperiod,P^RM“(theconstant expect forasymptoticallysmallamplitudes).Asimple (Alexander andBudding1979),assuminganorbital colors atmaximum(ArpandHartwick1971),binary erable extrapolationisrequiredtotheepochofobserva- from thesystemicvelocity.ThevelocityofV3NGC secondary minimumandthusshoulddiffernegligibly ties arenegligibleattheshortperiodsencounteredhere. safely assumethattheabsorptionspectrumarisesfrom ation inradius,say8B~8L/L~8R/R(asonemight companion. Thismodelisconsistentwiththeobserved main-sequence starwitha0.3Mlobe-fillinggiant the moremassivecomponentandthatorbitaleccentrici- amplitude ofavariableinsomebandpassislinearly sumption thatthespectrumoriginatesfroma1.4M tion, butitscorrectnesshasbeenassumedhere.The period variables,CW(WVirginis)typeclustercepheids, variables areincludedinthecatalogforwhich vated inlargemeasurebythefailureoflesssignifi- ity data,phasecorrectionswereestimatedbysimple variables ofthesetypeshavingonlyfragmentaryveloc- is well-established.ThesearetheM(Mira)typelong- components inanyofthefittedcurves. cant includedtermstointroduceobviouslyspurious relaxed significancecriteriaadoptedaboveweremoti- (dwarf cepheid)variables,andeclipsingbinaries.For age todefinetheradialvelocitycurve,butwhichbelong observations areinsufficientinnumberorphasecover- eye-interpolation ofthevelocitycurve.Indeed,very same typetodefinestandardvelocitycurves. scaling procedures,usingwell-observedfieldstarsofthe RR LyraestarsofbothRRabandRRctypes,RRs to atypeofvariablewhosecharacteristicvelocitycurve b 0 0 The eclipsingbinariespresentfewproblems.Wemay For pulsatingstars,thefollowingverysimplescheme Variables withfragmentaryvelocitycurves.—Many l/3, 8ü~^Mp-«B (7) r 198lApJS ... 45. .259W from thecalculationofstellar y-velocity,shownasathinhorizontalline. Radii ofthedatapointsinthese plotsreflectlogarithmicallytherelativeweightsassignedtothem. Opencirclesdenotevelocitiesomitted Fig. 1.—(a-J)Least-squaresFourierfitstotheradialvelocitycurves of10clustervariablesshowingdefiniteperiodicvelocitystructure. © American Astronomical Society •Provided by theNASA Astrophysics DataSystem 0.0 01.0 0.0 01.0 4> 198lApJS ... 45. .259W © American Astronomical Society •Provided by theNASA Astrophysics DataSystem a V78 NGC5139 V95 NGC5272 V6 NGC5139 VI NGC5139 V42 NGC5904 V154 NGC5272 V2 NGC6254 V2 NGC6205 V84 NGC5904 Vil NGC7089 Emission lines. Variable Fourier ComponentsofRadialVelocitiesClusterVariables —149.70±0.32 -150.09 ±0.53 + 208.8±1.9 + 52.70±0.66 + 213.6±3.7 -248.7 ±2.5 — 93.4±2.6 + 55.1±1.0 + 60.5±6.3 -7.4 ±2.0 TABLE 2 —17.7± 1.5 —11.8± 1.4 — 3.17±1.50 +0.36 ±1.20 +4.51 ±1.15 — 7.40±1.83 +4.54± 1.92 —0.39±0.60 —10.1 ±4.1 + 75.3±7.7 —17.6±7.5 —16.6±3.9 + 5.62±1.05 +2.92 ±0.96 + 12.4±3.4 — 0.2±2.8 — 0.2±1.6 ±2.9±3.4 — 11.34± -14.51 ± — 5.81± — 41.4± — 7.63± —2.06± — 9.67± +2.47± -0.21 ± — 37.9±12.5 —10.7 ± + 9.5± -9.0± — 5.9± + 8.6± + 5.7± — 2.4±2.9 — 0.2±2.6 0.98 0.85 0.60 0.44 4.4 2.5 0.94 0.98 5.4 7.5 3.7 1.5 1.6 1.69 1.10 198lApJS ... 45. .259W ü'(^)={ü(«f.)-a} brightness intime. phase, Listhetime-aVeragedmeanbrightness,and velocity isaconvolutionofradialwithapparent because theapparentbrightnessofsourceisalso is thenanintegralofthevelocitycurveoverphase,but plitude, AR,ofavariablecertaintype,itsvelocity equal intervalsofphasedonotcontributeequallytothe residual velocities,estimated byappropriatescalingof where t/andi/arethe maximumandminimum Here L(<¡>)istheapparentbrightnessasafunctionof with thelightcurvesforthesevariables).Asamatterof observed velocity.Totheextentthatvariationsofspec- correlated withphaseandhenceradialvelocity, ever, exposuresfrequentlyintegrateoverasignificant period. Theadoptedphasecorrectionisthenmerely velocity ofthevariable. curve definedbyawell-observedreferencevariableof curve canbeestimatedbyscalingthestandardvelocity tral typewithphasemaybeneglected,theobserved fraction ofaphotometricperiod.Theobservedvelocity exposures areshortcomparedwiththephotometric where istheresidual(apparentminusstellar) gether minor.Then,giventheperiod,P,andam- (compare Eggen1951;TifftandSmith1958;Femie by alinearmappingofthevelocitycurve: example, thevelocitycurvesreproducedinFig.2,below, the sametype: among clustermembers,differencesofmasstobealto- the referencevelocitycurve (eq. [8]).Thenthemeasured expedience then,thelightcurvemaybeapproximated curves arevirtualinversionsofeachother(compare,for 0var tors, itiswellknownthatthelightcurvesandvelocity 1965; WoolleyandAly1966).Oneexpects,certainly 0 var maxin var d d Among theshorterperiodvariables(Pl),spectral © American Astronomical Society •Provided by theNASA Astrophysics DataSystem ß=- L(= —t/(<í>).(9) 04AZ? 1-10“ A Aß ref -0.4A5 / RADIAL VELOCITIESINGLOBULARCLUSTERS 1/ rr <0, (11) (8) Theadoptedphasecorrectionisthen d 1 velocity foralongintegrationis periods], orexposuresofanintegralnumberperiods, (Note thatforverylongexposures[manyphotometric lines (exceptHy,Hö,Hf,andMgnA4481).Thephases midpoint intheascenttophotometricmaximum,re- mean curveprobablyarisesfromrealcycle-to-cyclevari- ments; mostofthedispersionthesepointsabout Joy’s classicstudy(Joy1926).Figure2aillustratesthe As inTable2,Fouriercomponentslisteditalics itself [seebelow]yieldsanestimatedsystematicdif- once: forV9NGC104,V12 NGC104,andV65 curve alsovarywiththisperiod.Thevelocity (the Blazhkoeffect);thelightamplitudeandvelocity errors. InthecaseofRRLyrae,phase curve foroCeti(Mira)wasfittedtothenormalpointsin Table 3arethosewhoseinclusionisnotsignificantata reference velocitycurvesarelistedinTable3,withtheir example, integrationthroughafullperiodofRRLyrae cally negativewithrespecttothetruestellarvelocity.For RRc, andRRsvariableswere eachemployedhereonly zero phasetophotometricmaximum (seeSanford1949; corrected fortheBlazhkoeffectgiveninthatpaperwere adopted hereisafittolongseriesofmeasurementsby ferred toaconstantephemeris,varieswith41period ations (cf.Joy1954),ratherthanfrommeasurement fit ofthisreferencecurvetoJoy’sindividualmeasure- formity inphasecoverageoftheirvelocitycurves.The Fourier coefficients,andillustratedinFigures2a-2e. ference of—6.8kms“.) 5139, respectively. Gordon andKron1947).The referencecurvesforRRab, Struve andBlaauw(1948)ofthemeanvelocitiesall selected onthebasisofextent,accuracy,anduni- 90% confidencelevel.Thesereferencevariableswere Since ßisnegative,themeasuredvelocitiesaresystemati- adopted, butcorrectedalsobyA=—0.366torefer The variablesactuallyemployedheretoestablishthe ^obs -a + 0 2 a2 rv()L()d )). (14) •'<¡>1 2,d ß rv'(i>)4>+ A«=-(t3-a) (13) obs0 a i J =0 applied,togiveanestimate ofthestellary-velocity. been correctedto<#>=0,the displacementcorrection present catalog.Ingeneral,whenthephaseofanob- This relationship,withastandarderrorof±5.2km applied, andthentheabsorption-line phasecorrectionat servation isknown,theemission-line velocityhasfirst s (independentofperiod),hasbeenadoptedinthe where Pisthepulsationperiodindays,andveloci- ties areatphotometricphase<¿>=0(maximumlight). find thatthiscorrelationiswellapproximatedby e.g., Merrill1941;Feast1963).SmakandPreston(1965) displacement iscorrelatedwithpulsationperiod(see, variables aresystematicallyblueshiftedwithrespectto the absorption-linesystem,andthatamountofthis velocities atmaximumaresystematicallyredshiftedwith longer periodvariables(P>300),theabsorption-line been adoptedasmeasuresofstellarvelocityforthe ies, thattheabsorption-linevelocitiesatmaximum variables cataloguedhere. respect tothestellarvelocitiesgivenbycircumstellar correspond tothestellarvelocity.However,Reidand Dickinson (1976)havesinceshownthat,atleastamong tion-line y-velocitiesofthesestars,whichhavetherefore OH maseremission.Wenoteherethattheveloci- ties areingoodagreementwithestimatesoftheabsorp- -13.93 = -16.20= -13.46 = +0.44= + 5.461 -5.67 = -7.09= -4.75 = -6.57 = -2.04 = -3.77 = -7.42 = -1.50 = -3.00= -7:30= -2.07 = + 2.66= It iswellknownthattheemissionlinesofMira-type :0.75 :0.74 : 1.37 : 1.14 :0.42 :0.43 :0.42 :0.43 :0.40 :0.62 10.62 :0.59 :0.60 :0.54 :0.34 :0.13 :0.13 , «ab(0)-t=e(0)=0.035i>kms- (17) Sm) ii) Emission-LineDisplacements(a) -10.35 = -19.72 = -3.04= -0.90 = + 2.50= + 0.72= -1.33 = + 0.52= + 2.48= + 1.51= -0.30 = + 3.09= + 0.11= -1.38 = -6.88 = + 0.69= -4.96 = :0.72 :0.73 :0.91 :0.97 :0.43 :0.43 :0.43 :0.42 :0.45 .0.61 :0.60 :0.60 :0.56 :0.40 :0.49 :0.15 :0.12 Joy (1926) Joy (1926) Van Citters(1976) Jacobsen (1929) Epps andSinclair Struve andBlaauw (1973) (1948) Reference 269 198lApJS ... 45. .259W -1 d -1 -1 -1 -1 -1 previously publishedvelocityincolumn(4).Gunnand published hisownvelocitiesforthefirsttime,dif- ously publishedvalues.Inthesecases,whereZinnhas differences betweenhisownmeasurementsandprevi- number ofstarsinNGC5272withrespecttotheir ference aspublishedappearsincolumn(3),withthe A 5=4.0havebeenassumed,asthesevaluesaremore cluster velocity,fixedat—146.9kms(col.[4]). ity. log. Ingeneral,however,littleornothingisknownof have alsobeenpublishedandareincludedinthecata- are missingfromHogg’s(1973)catalog,P=200and Griffin (1979)giveresidualvelocities(col.[3])foralarge velocity ofthereferencestarorcluster,asdeterminedin typical ofglobularclusterMiravariables. may bebroadlycharacterizedasfollows: presentation ortreatmentofthedata.Theseinstances give geocentricvelocitiesofthreestars. Eridanus cluster,forwhichWestandBartaya(1979) apparent. Ithasbeennecessary,therefore,toexclude cases wheretheyappearedwarrantedbytheoriginal these velocitiesfromdeterminationofthestellarveloc- the caseofV6NGC5139somephasestructureis their behaviorinthestellarreferenceframe,although 270 the presentcatalog,andthatadoptedinsourcefor which weobtainavelocity+83.8±1.5kms,in ROA 70inthesamecluster.Weobtainhereameanof of ROA153inNGC5139tothemean55and Hesser andShawl(1977)quoteavelocityforNGC6441 observations ofHarding(1962)andDickens(1972). the velocity.SmithandWing(1973)referredvelocities measured differentiallywithrespecttoNGC6388,for excellent agreementwiththeirvalueof+81kms and Freeman(1979)obtained velocitiesofV78NGC adopted fromKinman(1959).Finally,Lichten,Liller, correlation withROA24in thatcluster,forwhichwe 5139 attheAnglo-Australian Telescopeviacross- derive avelocityof+236.3+4.2 kmsversus+234 -1-215.2±7.9 kmsforthesetwostars,basedonthe + 15kmsquotedbyHarding (1965). Zinn (1974)haspresentedvelocitiesofafewstarsas These haveprovednecessaryonlyinthecaseof Emission-line velocitiesofafewothervariablestars The valuequotedisthedifferencebetweenrevised Zero-point correctionshavebeenappliedinthose © American Astronomical Society •Provided by theNASA Astrophysics DataSystem i) VelocitiesReferredtoaFixedNonzeroVelocity ii) VelocitiesReferredtoAnotherStarorCluster b) HeliocentricCorrections(h) c) Zero-PointCorrections(r) WEBBINK 1 -1 -1 1 -1 -1 -1 -1 _1 NGC 6205,6341and7078inordertoobtainconformity individual starswithothermeasurementsoftheself-same with Kinman’s(1959)velocitiesfortheseclusters.These rated inthepublishedvelocities.NorrisandZinn(1977) was notedbytheauthorofpublishedvelocities.Van rived fromallindependentdata.Therevisionstothe corrections havebeenrecalculatedhereonthebasisof applied suchcorrectionstotheirstellarvelocitiesin ual stars,plustheclustervelocity). (from 12individualstars,plustheclustervelocity),and 6205 (bycomparisonofthreeindividualstars,plusthe corrections employedbyNorrisandZinn(correctionsto independent determinations.Hestatesthatasystematic den Bergh(1969)measuredvelocitiesfromintegrated cluster velocity),—3.9+10.2kms“forNGC6341 stars andweightedvelocitieswithclusterde- all othermaterialavailable,comparingbothvelocitiesof spectra of22galacticglobularclusters,which19have the corrections)amountto—6.9±7.5kmsforNGC published velocitiesquotedincolumn(3).Ineachin- difference hasbeenredeterminedonthebasisofall difference of+19+7kmswasfoundintheob- applied asasystematiccorrection. s “(catalogminusvandenBergh),whichhasthenbeen available material,forwhichweobtain+13.4+6.3km the oppositesigntothisdifferencewasintended.This served minuscatalogradialvelocities,butitisclearthat with k=\0.2kms,where fisthezenithdistanceof in column(4)ofthecatalogarecorrectionsto cliffe Observatory(reciprocaldispersions86Âmm radial velocitystandards,andthoseobtainedwiththed difference betweenvelocitiesobtainedwiththeccamera observed. FeastandThackeray(1963)foundthatthe errors dependentonthezenithdistanceofobject values astheywereoriginallymeasured. the staronmeridian,measured southward: camera canbeexpressedas (49 ÁmmatH),whichareingoodagreementwith and 170Àmm,respectively,atH)showsystematic differences merelyrestorethevelocitiestoheliocentric quoted inthecatalog.Incase(i),ofcourse,zero-point stance, save(i),theuncertaintyinsystematiccorrec- tion isincorporatedinthestandarderrors(col.[5]) — 11.7+2.9kmsforNGC7078(fromtwoindivid- y y In somecaseszero-pointcorrectionswereincorpo- In oneothercasetheappearanceofazero-pointerror Velocities obtainedwiththedandecamerasatRad- The zero-pointcorrectionsderivedhereandquoted o iii) AbsoluteVelocitieswithKnownZero-PointErrors d) ZenithCorrections(z) Av(c—d) =ktanÇ,(18) ?=«<>-«> (19) Vol. 45 198lApJS ... 45. .259W where ô=—25°273isthelatitudeofRadcliffeOb- zenith correctionbutultimatelyrejecteditonthe east ofthepier;signthiscorrectionshould servatory. (Itisassumedthroughoutherethatforthe otherwise bereversed.)Harding(1965)laterfoundno few clustersnorthofzeniththetelescopewas[asusual] No. 2,1981 so thattheecameravelocitiesareapparentlysimilarly systematic differencebetweeneanddcameravelocities, velocities Kinman(1959)obtained withthedcamerafromin- velocities withlinearlyindependentfromother grounds thatintegratedspectrashouldberelativelyun- affected. clusters wheresuchacomparisonispossible.Filledcirclesindicate distance, I(positivesouthward),atRadcliffeObservatory,for15 have beenaffected(Fig.3).Aweightedlinearleast- possible showsthatbothintegratedandstellarspectra cerned betweenstellarandintegratedvelocitieswithin derived byFeastandThackeray (1963) withthesamecamera. dependence ontanf.Thedotted lineisthezenithcorrection and stellarspectra.Theresiduals showastatisticallysignificant affected, whereasnosystematicdifferencecouldbedis- sources for15clusterswheresuchacomparisonis the sameclusters.However,acomparisonofKinman’s and partiallyclosedcirclesthose fromcombinationsofintegrated tegrated spectra,opencirclesthose fromindividualstellarspectra, squares fittothevelocitydifferences(independent— 0 Kinman (1959)discussedthepossibleneedfora Fig. 3.—Residualvelocities,At;(others—Kinman),vs.zenith © American Astronomical Society •Provided by theNASA Astrophysics DataSystem RADIAL VELOCITIESINGLOBULARCLUSTERS -1 2- be relievedinsomemeasurebytheadoptionofsuitable were morerealisticallyassessed.Thisshortcomingcan difficulties, themostobviousofwhichisatendencyto square oftheirstatedstandarderrorsinvolvesserious rejection criteria(§IVcbelow),bywhichcertaindata favor thosedatainwhichtheerrorsareunderestimated, has beenincludedroutinelyinthepublishedvelocities. by theoriginalauthors.Sincethattime,thiscorrection velocities. Inmanycases, however, thedataaretoo velocities fromindividualstars,whereanirreducible extensive dataexistonagivenstarorcluster.Itisalso at theexpenseofhigherqualitydatainwhicherrors with thedandecamerasatRadcliffeObservatoryprior of NGC104;thesmalldifferencebetweenthiscorrec- of +10kmsinthedcameravelocitiesintheirstudy confidence levelandconsistentwiththecorrelation(eq. The dependenceonzenithangleissignificantata90% Kinman) asafunctionofzenithdistancegives limited forthesemeasures to sufficeincontrollingthe As discussedin§IIabove,standarderrorshavebeen therefore beenadopted. [9]) obtainedbyFeastandThackeray(1963),whichhas vidual measurements.The reader shouldthereforebe introduction ofspuriously highweightsforindi- duced inthevarianceassigned toindividualstellar are excludedentirelyincomputingthemean,where a—100 kmsasthestandardunitofvariance,they estimated foreachoftheentriesincatalog.The to 1965,exceptwhereithasbeenexplicitlyincorporated tion hasbeenappliedtoallothervelocitiesobtained above) hasbeenappliedhere.Ingeneral,thefullcorrec- tion andthatobtainedfromtheirlatercorrelation(given additional term(theclustervelocitydispersion)isintro- amehorated toagreatextentinthecalculationofcluster general philosophyhasthereforebeenfollowedbelow and requiresometreatmenttocompensateforthatfact. assigned byKinman(1959)tohismeans. assigned byKukarkin(1974)tohisclustervelocitiesand these weights(givenincol.[7]ofthecatalog)aregener- their expectedvariancefromthemean.Preciselyhow that individualvelocitiesshouldbeweightedinverselyas tire clustersareclearlyofveryheterogeneousquality are agoodapproximationtoone-tenththeweights are inprincipledirectlycomparablewiththeweights ated isdiscussedindetailbelow.Withthechoiceof Clearly, weightingmeasurementsinverselybythe Velocities availableforbothindividualstarsanden- Feast andThackeray(1960)incorporatedacorrection 1 Au (kms“)^-(4.5±2.3)+(15.5±3.9)tanf. IV. DETERMINATIONOFSTELLARANDCLUSTER VELOCITIES (20) 271 198lApJS...45-.259W 2- 1 - versely, whereveryextensivedataareavailable,the rejection criteriadetailedbelowtendtoensuresome data areprobablysystematicallyunderestimated.Con- rors. measure ofaccuracyintheassessmentstandarder- lar orclustervelocitiesbasedonveryfragmentary admonished thatthestandarderrorsassignedtostel- where, again,a=100kms.Whereanindividual 272 where is thedispersioninemission-linedisplacementcorre- where eisgivenbyequation(16)and_=5.2kms” line velocities velocities wereweightedasinequation(21).Inthe variable stars.Inthefirst,whereaFourierrepresenta- individual stellarvelocitiesaredecreasedbyafactorn: in thecluster(forexample,velocitiesofvZ612,752, velocity foragivenstarisdrawnfrommeannstars weighted meanstellarvelocitywasderived,weighting were weightedbyafactor unstable lightcurvesandwidestar-to-stardifferencesin lation (eq.[17]).Inthethirdcase,wherenophase velocities each (corrected)observationbytheinversesquareofits corrections couldbederived(whichisgenerallythecase where eisgivenbyequation(15);foremission-line standard error(inkms the formsoftheirvelocitycurves),individualvelocities among theRVTauristars,whichfrequentlyhavevery second, wherephasecorrectionswerederivedfroma the weightsassignedtomeanvelocityincomputing scaled referencevelocitycurve,wehaveforabsorption- tion ofthevelocitycurvecouldbecalculated,individual 1127, and1208inNGC5272fromSanford[1919a]), ea a When twoormorestellarvelocitieswereavailable,a Three casesmaybedistinguishedinthetreatmentof © American Astronomical Society •Provided by theNASA Astrophysics DataSystem 2 w(em)=a[ej +e_<.=0)](24) ic 2>_2/3 2 o=300i(Afi)knis “, (26) var 2 M/,(abs)=a(e,+e^) (23) a) StellarVelocities w^aiej +0^) (25) w,=a(/ie^) (22) Wi=a(ej) (21) WEBBINK 2 2 velocity dispersion.Forthe sakeofsimplicity,theesti- variance, a//m,inthecluster velocity,asdeducedfrom is ameasureofthetypicaldispersioninradialvelocities way ofaccomplishingthis,andthenominalerrorschar- integrated spectraarestilldominatedbyafinitenumber variance ofthevelocityfromsamplingstatistics,as is unknown,valuestypicalofothervariablesinthe the meanvelocityofmstars, whereoisthecluster the samplingerrorcanbe estimated andintroducesa available withoutindividual identifications.Inthiscase for samplingerrorstoproduceasignificantcontribu- of stars.Inpractice,however,thereisnostraightforward been assumed.Equation(26)isobviouslyonlyan of apulsatingvariable.Inmanycases,wherePorAB tion. acteristic ofintegratedspectraarerarelysmallenough In principleoneshouldincludeacontributiontothe variable stars. problems encounteredindefiningthevelocitiesofthese (T typicallyvariesbyfactorsof2to3fromobject order-of-magnitude estimate,aspulsationmodesand same areaoftheHertzsprung-Russelldiagramhave were computedasfollows: data, thisexpressionsufficestoreflecttheadditional object. Nevertheless,intheabsenceofmoreextensive gross physicalpropertiesofthesevariablesdifferwidely; mulae: standard errorarethencomputedbythefor- square standarderror: stellar velocities.Theweightsassignedtoeachofthese fied numberof(unidentified)stars,and(iii)individual of (i)integratedspectra,(ii)meanvelocitiesaspeci- c/ var In averyfewinstancesmeanvelocitiesofmstarsare The meanvelocityofnmeasurements(«>1)andits As above,velocitieswereweightedbytheinverse Cluster velocitiesarecomputedfromacombination ii) MeanVelocitiesofSeveralStars 2l- ^^«(e) kms.(29) b) ClusterVelocities i) IntegratedSpectra («-OSw, 1/2 Vol. 45 (28) (27) 198lApJS ... 45. .259W No. 2,1981 velocities arenotinfrequentlypresentinintegratedspec- ities. Pastexperienceshowsthatunaccountablyspurious of radialvelocitysoastominimizetheinfluence here fora.Wethereforeassignweight a, ratherthanatthestellarposition,hasbeenadopted velocities bydataofpoorerqualitythansignified pensation isdesirableagainstunduedominationofmean discrepant dataonthededucedstellarandclusterveloc- resolved. Furthermore,asdiscussedabove,somecom- of membershipindividualstarsarenotalwaysclearly bility: where eisthestandarderrorinstellarvelocity(eq. mated apparentvelocitydispersionattheclustercenter, not beestablished.Inaddition,thosevelocitiescorre- ment correctiontotheabsorption-liney-velocitycould tral data(e.g.,NGC6441,6838),whilequestions observation, notofthestellarvelocity,andwemustthen quoted incolumn(7)ofthecatalogisthatsingle [28]). Whereonlyonevelocityisavailable,theerror of V42NGC5904nearphase=0wereexcludedin ties ofindividualstarswererejectedwhenthedisplace- their nominalerrors. to thesevelocities. calculating itsvelocitycurve. sponding tothedoubledpeaksinabsorptionspectra here. were publishedbyStrömberg(1925)andarepreferred (1935), whichareweightedmeansofhisownand (1946) inpreferringthevelocitieslistedbyEdmondson allow explicitlyforanycontributionfromstellarvaria- R. F.Sanford’svelocities,obtainedatMountWilson, Slipher’s measurements.Similarly,revisionstosomeof Slipher atLowellObservatory,wehavefollowedMayall vidual stars,is,ofcourse, one ofmembershipinthe cluster velocities.Thefirst of these,applicabletoindi- certain datafromconsideration incomputingstellarand c) 0 It isusefultoexercisesomediscretionintheinclusion As discussedin§Ila(ii),certainemission-lineveloci- In thiscasewehave,ofcourse, Regarding theveryearlyspectraobtainedbyV.M. Two othercriteriahavebeen appliedheretoexclude © American Astronomical Society •Provided by theNASA Astrophysics DataSystem iii) IndividualStellarVelocities 2 2 c) RejectionCriteria w,=a|e +^-j(30) H',.=a(e+a) ',(31) 0 2 e=+a. (32) ar RADIAL VELOCITIESINGLOBULARCLUSTERS 2 2 have naturallybeenexcludedincomputingclusterveloc- both toindividualstellarvelocitymeasurements,and ities, ashavestarsforwhichtangibleevidenceexiststhat integrated spectra. where ëisthestandarderrorofmean(orphase- individual velocitiescomprisinganymean,withthesole velocities areinmanycasesclearlynon-Gaussian mean stellarvelocitiesofsupposedmemberstarsand cluster inquestion.Fieldstarsandprobablefield in column(2),andcentralescapevelocities [14]). Thesecondcriterionisastatisticalone,applied they arepossiblyfieldstars(indicatedby“mem?”incol. worth (1976)for10clusters fittoKingmodels.In mean valueoftheempirical ratiosobtainedbyIlling- neous Kingmodelsforthe clusterswithmass-to-fight dispersions, usedinweightingstellarvelocities,arefisted cataloged dataarelistedincolumn(4)ofTable4,with lously highweight. principle, therejectionofdiscrepantdataanoma- velocities satisfyit.Thisprocedureallows,atleastin rejected inthisway,themeanandstandarderrorare corrected) velocity,o,withthevelocityinquestion curves. Anymeasurementisrejectedwhichdoesnot exception ofvariablestarswithundefinedvelocity distribution. Axtesthasthereforebeenappliedtoall skew meanclustervelocities,buteventheremaining ties; unrecognizedfieldinterloperscan,ofcourse, ratios M/L—1.3M(O)/L (0), whichistheweighted compilation ofupdatedcluster data,adoptinghomoge- (3). Thesevalueswerecomputedfromanextensive has beenemployedhere.Ifthetrueerrorsare recomputed, andthextestrepeateduntilallremaining included inthesample.Ifoneormorevelocitiesare standard errorsincolumn(5).Apparentcentralvelocity velocity. Thisresultsfromtheweightingschemewhich racy ofthestandarderrorsassignedtoeachmean satisfy ing else,ensurethattheerrorsarenotfullyGaussian. Gaussian-distributed, weexpect of thestandarderror. of theconfidencewhichcanbeplacedineitherestimate obtained fromequation(28)maybeusedasameasure However, agreementbetweenthisestimateandthat Of course,therejectioncriteriaoutlinedabove,ifnoth- v Ü We seekthemostprobablestellarorclusterveloci- Weighted meanclustervelocitiesderivedfromthe A usefulcheckisultimatelyprovidedontheaccu- 2 X=(ü,-t))^;+ê| <4,(33) V. CLUSTERVELOCITIES 2 <8>«a(2>,) (34) 273 198lApJS ... 45. .259W NGC 288 NGC 1261 NGC 362 NGC 104 NGC 6293 NGC 6284 NGC 6273 NGC 3201 NGC 2808 NGC 2298 NGC 1904 NGC 1851 NGC 6341 NGC 6333 NGC 6304 NGC 5694 NGC 5466 NGC 5024 NGC 4833 NGC 4372 NGC 4147 NGC 2419 Cluster NGC 6397 NGC 6362 NGC 6356 NGC 6205 NGC 6121 NGC 5904 NGC 5634 NGC 5286 NGC 5272 NGC 5139 NGC 4590 Pal 3 Pal 2 Pal 1 NGC 6388 NGC 6229 NGC 6171 NGC 6139 NGC 6093 NGC 5986 NGC 5927 NGC 5824 Pal 4 Eridanus NGC 6266 NGC 6254 NGC 6218 Pal 14 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem 10.60 11.63 12.06 13.51 10.07 17.42 13.50 0.96 5.19 9.45 2.71 4.35 3.97 7.90 6.45 6.64 6.33 6.15 4.42 4.30 0.83 3.23 9.44 7.68 9.25 5.25 2.39 8.86 3.15 3.55 2.88 4.71 5.76 5.31 3.39 4.79 7.00 6.73 6.74 6.11 5.59 5.22 5.67 4.22 1.10 1.10 7.10 7.85 1.22 7.19 Cluster RadialVelocities 41.79 26.10 26.13 45.36 55.29 38.29 49.87 30.53 32.49 25.80 26.71 24.70 39.12 71.32 28.42 47.95 36.28 29.01 21.12 23.06 21.03 19.80 38.27 27.23 28.17 21.33 18.32 12.21 54.27 20.56 22.04 28.41 32.12 13.09 11.35 16.99 14.39 17.21 12.66 17.67 18.72 16.14 13.36 esc 4.33 9.78 8.85 3.79 4.06 2.97 3.41 TABLE 4 274 +121 +224.7 + 22 +182 + 55 +119.9 + 48.6 +228.3 +216.6 + 83 +168 +494.0 +104.1 +185.4 +318.6 +232.4 + 19.0 + 83.8 + 31.6 + 7.6 + 64.3 + 81.0 + 51.9 + 22 + 44 + 3 - 73 + 12.9 - 48.2 -120.5 - 98 + 70.1 - 78.9 -116.5 - 6.2 -133 - 35 - 58 - 63 -147.11 - 20 - 40.5 - 14.10 - 60.9 -154.2 -247.8 -147 - 78 -183.8 - 43.5 57 57 28 32 10 11 12 15 13 32 11 10 14 11 12 12 17 16 5.0 7.5 8.0 4.4 0.94 8.2 4.6 0.47 4.6 5.0 9.7 2.8 2.5 6.0 7.8 6.9 2.7 2.9 6.9 7.5 1.7 1.7 4.3 3.2 7.6 2.3 6.1 2.8 2.4 1.5 1.1 1.7 118 41 89 36 46 53 12 16 10 16 4 3 4 5 5 5 9 3 3 2 6 4 8 4 3 4 5 5 7 7 238.33 50.83 32.57 29.89 66.96 35.87 11.26 27.51 15.20 13.87 11.00 18.26 10.22 Wt 0.82 4.14 0.03 0.57 0.38 0.97 0.03 0.12 0.38 0.18 7.24 0.96 0.38 0.51 0.38 0.38 0.47 0.28 8.47 2.57 2.95 7.61 6.83 0.18 0.60 0.38 1.37 1.14 0.38 8.25 1.48 7.65 7.99 2.20 1.53 1.71 1.66 198lApJS ... 45. .259W NGC 6440 NGC 6402 NGC 6541 NGC 6528 NGC 6522 NGC 6441 NGC 6553 NGC 6544 Cluster NGC 6624 NGC 6584 NGC 6638 NGC 6637 NGC 6626 NGC 6642 NGC 6652 NGC 6715 NGC 6712 NGC 6681 NGC 6656 NGC 6779 NGC 6723 NGC 6809 NGC 6752 NGC 6864 NGC 6838 Draco Ursa Minor NGC 7492 NGC 7099 NGC 7089 NGC 6934 Pal 11 Pal 12 NGC 7078 NGC 7006 NGC 6981 Fornax Pal 13 Sculptor © American Astronomical Society •Provided by theNASA Astrophysics DataSystem 13.54 14.28 12.89 0.55 4.77 4.59 7.88 6.86 1.27 1.03 1.11 1.73 9.87 8.75 8.23 4.56 4.21 8.17 6.06 4.50 8.42 6.12 6.97 9.39 6.12 3.18 4.67 4.52 5.60 5.37 6.99 3.93 3.29 6.05 9.16 2.88 7.97 4.45 1.66 Dwarf SpheroidalSystems 20.40 23.49 33.05 15.44 57.24 36.38 23.61 34.05 57.99 35.12 32.69 26.78 27.47 33.70 16.77 35.43 25.46 17.52 53.56 29.99 20.11 12.71 17.19 23.02 17.31 4.58 37.66 5.78 3.96 35.06 23.30 10.83 3.80 15.53 17.08 1.97 17.19 12.32 5.69 TABLE 4—Continued + 51. +196 + 9 - 28 -278 -244 -188.5 -172.3 - 6.1 275 + 8 + 13.9 +101 + 69 +180 - 84 -123.4 -152.8 - 12.0 +198 - 32.6 + 35 +131.0 +166.6 -123.9 -152.5 -138.1 - 32.2 -278 - 68 -195.2 - 19.27 -384.8 -379 -112.1 124.2 50.1 90 14 1.8 37 35 80 34 23 50 32 16 11 12 11 14 15 15 2.9 3.3 10 8.5 8.2 12 13 5.3 3.1 3.4 7.8 6.0 7.1 6.2 7.1 3.7 4.9 2.6 0.92 7.6 3.2 4.4 4.4 7.3 1.9 16 10 29 42 2 14 2 2 5 8 4 5 6 7 3 4 6 8 7 6 11.57 13.02 15.26 94.89 13.39 0.12 0.31 0.19 3.03 0.02 0.12 0.12 19.62 Vt 0.38 5.29 3.37 7.69 0.38 0.15 0.75 1.78 1.81 1.13 0.38 0.38 0.83 0.47 5.16 1.18 8.26 5.42 4.48 0.30 8.85 1.07 0.47 6.76 1.67 1.11 198lApJS ... 45. .259W 276 columns (6)and(7)thetotalnumberofvelocities(in- NGC 6522liesinBaade’swindowandisheavilycon- cluster velocities. and theirtotalweights.Asdescribedabove,thisaffords tegrated plusstellar)contributingtothemeanaregiven, The quotedvelocityisaweightedmeansatisfyingequa- a measureoftheconfidencewhichcanbeplacedin able forthisclustershowanapparentbimodaldistribu- taminated byfieldstars.Thefewvelocitiesavail- disturbing numberofsuchinstanceshaveoccurredin tion (33),butitisratherlikelythatthetruevelocitylies tion, withneitherpeakclearlyfavoredovertheother. interferometric radialvelocitysurveyofHesserand Table 3restonahandfulofobservationsbysingle tainly notfreefromlargeaccidentalerrors.Clearlya observer. Indeed,provisionalresultsfromtheextensive the past,andagoodmanyofvelocitieslistedin ±2e fromthismean. Shawl indicatethatsubstantialcorrections,exceeding .1974,Astr.Ap.Suppl.,13,345. .1931,Pub.YerkesObs.,6,1. .1977a,Astr.Ap.Suppl.,29,383. .1976,Astr.Ap.Suppl.,26,251. .1975c,Astr.Ap.Suppl.,22,193. .19756,Astr.Ap.Suppl.,21,15. .1975a,Astr.Ap.Suppl.,21,5. .\913,AtlasofGalacticGlobularClusterswithColourMag- .1955,Ap.J.,122,146. .1935,Ap.J.,82,396. .1958,T./.,63,118. .1957,A.J.,62,129. .19556,A.J.,60,317. .19776,Astr.Ap.Suppl.,29,397. Abt, H.A.1955,Ap.J.,122,72. .1962,Ap.J.,135,311. Alcaino, G.1970,Ap.7.,159,325. Barnes, S.A.1968,J.,73,579. Barnard, E.1914,Ap.J.,40,173. Barbon, R.1965,Contr.AsiagoObs.,No.175. Artiukhina, N.M.1956,TrudyAstr.Inst.Shternberga,21,3. Arp, H.C,andJohnson,L.1955,Ap.J.,122,171. Arp, H.C,andHartwick,F.D.A.1971,Ap.J.,167,499. Arp, H.C.1955a,A.J.,60,1. Andrews, P.J.,Feast,M.W.,LloydEvans,T.,Thackeray,A.D., Alexander, M.E.,andBudding,E.1979,Astr.Ap.,73,227. Cannon, R.D.1974,M.N.R.A.S., 167,551. Burbidge, G.,andSandage,A.1958, Ap.J.,127,527. Brown, A.1951,Ap.J.,113,344. Bohlin, K.1906,Astr.Fakt.StockholmsObs.,8,No.3. Belserene, E.P.1959,A.J.,64,58. Baum, W.A.1954,A.J.,59,422. Arp, H.C,andMelbourne,W.C.1959,A.J.,64,28. Arp, H.,Brueckel,F.,andLourens,J.v.B.1963,Ap.J.,137,228. Arp, H.C,Baum,W.A.,andSàndage,A.R.1953,A.J.,58,4. Cannon, A.J.,andMayall,M.W. 1949,Ann.HarvardObs.,112,1. Bond, H.E.1975,Ap.J.{Letters), 202,L47. Bailey, S.I.1902,Ann.HarvardObs.,38,1. Baade, W.,andSwope,H.1961,T./.,66,300. Baade, W.1926,Mitt.HamburgerSternw.,6,61. The velocityofoneclusterdeservesspecialcomment. 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(see Alcaino1973). 3d edition(Moscow:Akad.NaukS.S.S.R.,Astr.Soviet). P. Fedorov(Kiev:NaukovaDumka),p.118. Mat. Nat.,10,136. Globular Clusters,Cambridge,England. 1534. 119. 1216. 277 198lApJS ... 45. .259W 278 .19196,CarnegieInst.YearBook,18,249. .1949,Ap.J.,109,208. .1919a,Pop.Astr.,27,99. .1919,CarnegieInst.YearBook,18,249. .1924,Pop.Astr.,32,622. .1922,Pop.Astr.,30,9. Sanford, R.F.1918,CarnegieInst.YearBook,17,213. Slipher, V.M.1918,Pop.Astr.,26,8;Pub.AAS,3,331. Shilow, M.1898,Bull.Acad.Imp.Sei.St.Petersbourg,ser.5,8, Searle, L.,andRodgers,A.W.1966,Ap.J.,143,809. Schlesinger, F.1934,A.J.,43,97. Scheiner, J.1892,Abh.K.Preuss.Akad.Wiss.,Math.Abh.,1892. Sawyer, H.B.1955,Pub.DavidDunlapObs.,2,33. Savedoff, M.P.1956,A.J.,61,254. Sargent, W.L.1967,Ap.J.{Letters),148,L147. Sandage, A.,andWildey,R.1967,Ap.J.,150,409. Stoeckly, R.,andGreenstein,J.L.1968,Ap.J.,154,909. Stephenson, J.B.1961,A.J.,66,85. Smith, M.G.,andWing,R.F.1973,Pub.A.S.P.,85,659. Smak, J.I.,andPreston,G.W.1965,Ap.J.,142,943. Simoda, M.,andTanikawa,K.1970,Pub.Astr.Soc.Japan,22, Schultz, H.1886,BihangtillK.SvenskaVet.Akad.Handlingar, Sanders, W.L.1971,Astr.Ap.,15,173. Sandage, A.,Smith,L.L.,andNorton,R.H.1966,Ap.J.,144, Stetson, P.B.1979,A.J.,84,1149. Smith, M.G.,Hesser,J.E.andShawl,S.1976,Ap.J.,206,66. Sandage, A.,andWalker,M.F.1966,Ap.J.,143,313. R. F.Webbink:DepartmentofAstronomy,341AstronomyBuilding,1011WestSpringfield,University Illinois, Urbana, IL61801 253. Bd. 12,Afd.I,No.2. 894. 143. © American Astronomical Society •Provided by theNASA Astrophysics DataSystem WEBBINK .1971,Astr.Ap.,14,111. .19586,Ap.J.,128,583. Van Gitters,G.W.,Jr.1976,A.J.,81,766. .19736,Astr.Ap.,25,409. .1959,Ap.J.,129,356. van Maanen,A.1927,Ap.J.,66,89. van denBergh,S.1969,Ap.J.Suppl.,19,145. van Agt,S.1967,Bull.Astr.Inst.Netherlands,19,275. Tifft, W.G.,andSmith,H.J.1958,Ap.J.,Ill,591. .1974,Ap.J.,193,593. Zhukov, L.V.1971,TrudyPulkovoObs.,ser.2,78,160. Woolley, R.v.d.1966,RoyalObs.Ann.,No.2. Wildey, R.L.1961,Ap.J.,133,430. Whitford, A.E.1960,A.J.,65,531. Wallerstein, G.1958aAp.J.,128,141. von Zeipel,H.1908,Ann.Obs.Paris,Mem.,25,FI. Strom, S.E.,K.M.,Rood,R.T.,andIben,I.Jr.1970,Astr. Strom, S.E.,andK.M.1970,Ap.J.,159,195. Zinn, R.J.,Newell,F.B.,andGibson,J.B.1972,Astr.Ap.,18, Zinn, R.,andDahn,C.1976,A.J.,81,527. Zinn, R.1973a,Ap.J.,182,183. Woolley, R.v.d.R.,Alexander,J.B.,Mather,L.andEpps,E. Woolley, R.v.d.R.,andAly,K.1966,RoyalObs.Bull.,No.114. Wilson, O.C.,andCoffeen,M.F.1954,Ap.J.,119,197. West, R.M.,andBartaya,A.1979,Astr.Ap.Suppl.,38,69. Swope, H.H.,andGreenbaum,I.1952,A.J.,57,83. Struve, O.,andBlaauw,A.1948,ApJ.,108,60. Stromberg, G.1925,Ap.J.,61,353. Ap., 8,243. 390. 1961, RoyalObs.Bull.,No.43. CATALOG OF RADIAL VELOCITIES IN GALACTIC GLOBULAR CLUSTERS

© American Astronomical Society • Provided by the NASA Astrophysics Data System 198lApJS ... 45. .259W R 4 NGC 104(47Tue) R 11 R 7 R 6 R 3 R 1 Primary IDAlt R 10 R 8 R 14 R 12 R 15 R 13 R 19 R 18 R 16 Int R 22 R 21 R 24 R 23 R 51 R 26 R 52 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem V 19 V 16 Lee 4715 Wy 197 Lee 3758 Wy 254 + 2.4 + 0.4 - 24 - 22 + 6.8 - 18.5 - 13.4 - 27 - 10.2 - 13.3 - 28 - 21 - 20.4 - 24.2 - 14.0 - 17.2 - 4.5 - 18.1 - 15.8 - 9.5 - 14.7 - 12.8 - 14.8 - 25.2 - 20.8 - 22.4 - 20.2 - 10.5 - 13.2 - 17.3 - 4.1 - 6.0 - 10.0 - 25.8 - 22.3 - 15.81 - 5.8 - 10.8 - 23.3 - 5.9 - 1.8 - 18.1 - 29.0 - 31.1 - 4.5 - 18.8 - 17.4 - 15.4 - 29.6 - 13.1 - 14.0 - 13.5 + 11 + 11 + 11 + 11 + 11 + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z + 0.8z Av 4.9 4.9 R 4.9 4.9 4.9 4.9 2.7 4.9 4.9 4.9 4.9 4.9 4.9 4.9 8 4.9 R 4.9 R 4.9 2.2 8.8 2.4 3 4.9 4.9 R 4.9 2.7 3.8 5 5 4.9 4.9 8.8 3.7 6.5 9.1 3 6.5 6.5 6.5 6.5 6.5 6.5 7.6 0.54 6.5 R 6.5 6.5 6.5 R 6.5 R 6.5 6.5 6.5 Ref Kin Kin Kin Kin K in 4.20 4.20 4.20 4.20 4.20 4.20 4.20 4.20 4.20 4.20 4.20 3.24 3.24 2.39 2.39 7.10 2.39 2.04 4.20 2.39 2.39 2.39 3.24 2.39 2.39 Wt 11.1 11.1 4.00 4.00 1.56 0.70 0.71 0.46 0.63 0.71 0.47 0.57 0.67 0.70 0.63 0.57 0.52 0.63 0.74 0.57 0.62 0.47 0.63 0.57 0.57 0.63 280 KL IIR K3 IIIR KL IIR K3 IIR KO II-IIIR KO IIIR B8 III:R M R G8 IIIR G8 III:R K4 II-IIIR KL IIR KL-2 IIIR M2 II-IIIR KO (III:)R K R KO III F8 VR K2 II G8 IIIR G8:(III): R G8 II-IIIR Sp Ref <11.36> 11.51 10.73: 11.76 11.77 +1.52+1.54Eg 11.42 +1.64+1.62Eg 11.76V +1.57+1.67Eg 11.97 +1.14Eg 11.74 LE 11.92 LE 11.50 12.29 +0.48-0.01Eg 11.03 +1.74Lee 11.74 B-V U-B RefRemarks LE LE LE LE LE LE =Lee 8745* =HHw 2027 fld* 198lApJS. LO R 79 NGC 104(Continued) Primary IDAlt R 58 R 8UBVphotoelectricphotometrybyEggen(1961)is R 22=HHw2028 R 18=HHw4041 R 16Field?(Eggen1961). Remarks: Lee 1518=ChB524 Ba b=HD2167=CPD-72°39 -CoD-72°22 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem V 1 Lee 2602+2 Lee 1518-5 V 12 V 2 V 8 V 7 V 3 V 9 V 5 Ba b apparently ofthewrongstar. + 27.3 + 1.3 + 11 + 12 + 4 - 3.5 - 7.7 - 17.8e - 21.5e - 14.17 - 34.9e - 44.1e - 37.0 - 5.0e - 4.8e - 6.8 - 6.8 - 6.8 - 7.0 - 19.0e - 2.9 - 13.6 - 15.7e - 8.9 - 12.7e - 14.0e - 17.1e - 11.28 - 20.4+0.8z - 11.0+0.8z - 8 - 23.1 - 25.8 - 7.7 - 15.3 - 23.7 - 47.2 - 43.0 - 40.1e - 40.1 - 12.2e - 2.8 - 14.5e - 18.4e - 17.3e - 37 - 37.8e - 14.6 - 46.0e - 41.8e + 0.8 + 7 + 29 + 23 4.2 4.3 4.2 4.0 0.2 Av 0.8 0.8 4.3 4.4 4.4 4.1 1.6 4.3 3.0 3.0 3.1 3.1 3.2 7.8 1.9 3.2 2.6 3.0 3.0 3.0 3.5 7.5 2.3 5.7 2.1 2.3 6.6 3.0 2.3 3.0 ap pz ap apz apz P apz ap ap ap ap ap ap ap ap ap P pz 15 pz 15 ap P P ap P P P P P P ap pz 15 ap ap P P P 13 11 4.9 4.9 4.9 4.9 4.9 4.9 4.9 4.9 4.9 4.9 6.5 4.9 4.9 0.35 4.9 4.9 4.9 4.9 4.9 4.9 4.9 4.9 4.9 4.9 4.9 1.3 4.9 4.9 4.9 4.9 4.9 4.9 6.5 0.97 6.5 R 6.5 R 6.7 6.5 6.5 4.9 6.5 4.9 2.7 6.5 6.5 Ref NC NC F TW FTW FTW 4.03 0.41 1.80 1.80 1.80 4.10 1.80 4.20 0.43 1.92 4.16 1.87 1.87 4.09 4.13 4.00 4.00 4.14 4.11 4.11 4.07 1.80 1.80 4.14 1.36 1.36 2.39 1.78 1.88 1.88 4.17 1.88 1.88 1.80 2.39 1.78 1.78 1.35 1.78 Wt 0.57 0.55 0.59 0.74 0.73 0.73 0.72 0.72 0.57 0.38 281 V 3 M2-3 Ib V 12 V 5 V 2 V 1 M2-3 II:R<11.86><+1.41> M2: R<11.78><+1.66> M2 II-IIIR<11.68><+1.63> M2-3 II-IbR Lee 2602 A5-A7 FTW A5 FTW K2 II M2-3 Il-IbR<11.51><+1.45> G8 V: KO III FO Sp Ref =HV 814 =HHw 3085 =Lee 8756 =CPD -72°36 =Ch C199 =CPD -72°38 FTW <13.90><+0.27> <11.59> <+1.42> <11.65> <+l.31> 13.06 +1.08 10.20 +0.68 11.71 12.00 +1.09 B-V +0.86 Lee +0.75 Lee U-B RefRemarks ABL ABL 0.5:=HV203 ABL ABL LE FTW 0.13-0.85fld?* ABL ABL ABL 0.54 0.11-0.32 0.93-1.23 0.54 0.6: 0.2: 0.91 0.19 0.05 0.92 0.97 0.93 0.93 0.91 0.30 0.20 0.17 0.02 0.91 0.19 0.05 0.05 0.05 0.92 0.88 0.88 0.02 0.02 0.01 0.01 0.97 0.97 0.93 0.91 0.20 0.12 0.07 mem, =HV199* =HV 198* =HV 197* =HHw 1053* -HV 810 =HV 294 =HV 201* =HHw 1007* fld, =WyY* 198lApJS. References: NGC 104(Continued) HHw Hesser&Hartwick(1977) FTW Feast,Thackeray,&Wesselink(1960) Ch Chun(1976) ABL Arp,Brueckel,&Lourens(1963) Primary IDAltAveRefWt Ao Ao 213 Ao 96 NGC 288 Eg Eggen(1961b) Ba Bailey(1902) Ao 260 NGC 362 References: Reference: NGC 1261 Kin Reference: Kin Int Int HSt 2 HSt 3 Pal 1 HSt Reference: © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Alcaino (1975b) Kinman (1959) Kinman (1959) Hartwick &Sargent(1978) Kin 2 Kin 3 Kin 1 +218 +220 +238 +231 +201 +221 + 63 + 96 + 50 + 6 - 49 + 32 - 48 - 38 - 42.8 - 60 - 56.4 + 26 - 41 ■ 41 + 0 + 0 + 0 + 0 + 0 + 10 + 10 + 10 + 10 + 6 + 10 + 10 + 6 + 6 11 16 40 25 28 27 31 58 4 5 5.1 5 5.0 9 9 5 6 6 6 Kin Kin Kin Kin Kin Kin Kin Kin Kin Kin Kin Kin Kin Kin Kin Kin HSt HSt 1.23 2.78 4.00 4.00 282 1.13 3.02 3.09 1.23 2.78 2.78 0.83 6.25 0.10 0.030 0.39 0.14 0.16 0.12 0.062 Sp RefVB-VU-B NC Norris&Cottrell(1979) Lee (1977b) Wy Wildey(1961) R Feast&Thackeray(I960) LE LloydEvans(1974) Kin Kinman(1959) Kin Kinman (1959) 12.51 +1.89 12.96 +1.37 12.69 +1.58 Ref Remarks Ao Ao Ao [Radcliffe] 2 obs. 198lApJS ... 45. .259W Remarks: M Mayall(1946) NGC 1904(M79) Remarks: Int (a)RevisionbySlipher, basedonsame(b)Combinationof Slipher'srevisedvelocitywith Kin Kinman(1959) E Edmondson(1935) References: Int NGC 1851 Reference: WB West&Bartaya(1979) WB 3+2.6 HSt Hartwick&Sargent(1978) Pal 2_ WB 1-30.1 Int (a)RevisionbySlipher,basedon Reference: WB 2-31.0 Int Er Idanus(GCl0422-213) Int -13357HSt0.031 Primary IDAlt © American Astronomical Society •Provided by theNASA Astrophysics DataSystem plate asfirstentry. measurement ofsameplateby Edmondson. plate asfirstentry. +200 +178 +176 +252 +255 +168 +172 +245 +196 +206 +245 +235 +200 +320 +320 +309 +319 +277 +302 +295 +315 +300 + 13 - 0 - 0 - 0 - 0 - 17.9h 17.9 h17.2 17.9 h37.7 Av 12 12 13 16 19 23 33 33 33 33 37 37 19 19 23 37 37 9 9 5 6 6 9.6 WB M M M vdB Kin M M Kin Kin Kin E M M Sb Kin Kin Kin Kin SI E WB WB Ref Sb SI Wt 283 1.23 0.68 0.69 0.59 0.094 0.39 0.094 0.094 1.23 0.28 4.00 2.78 2.78 1.07 G8-KOIIIWB17.6+1.4 0.28 0.19 0.34 18.3+1.4 0.070 KO-K2IIIWB17.7+1.6 Sp SI Slipher(1924) Sb Strömberg(1925) (b) CombinationofSlipher'srevisedvelocitywith Ref remeasurement ofsameplatebyEdmondson. B-V U-B RefRemarks WB WB WB (b) (a) . (b) (a) 198lApJS ... 45. .259W M Mayall(1946) M Mayall(1946) NGC 2298 NGC 1904(Continued) NGC 2419 Reference: Kin Kinman(1959) E Edmondson(1935) References: Primary IDAltAveRefWtSpVB-VU-BRemarks References: Remarks: Reference: Kin Kinman(1959) E Edmondson(1935) Bd Baade(1935) Int +20 HSt 3 HSt 1 Pal 3^(SextansC) Int (a)MeasurementbyHumason. Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem +144 + 61 + 35 + 36 + 72 + 48 +113 + 85 +119 + 94 + 94 + 20 + 15 + 50 +103 - 30 - 25 - 53 - 20 - 5 + 13 + 13 13 45 40 HSt0.062 16 33 M0.094 33 M0.094 40 HSt0.062 11 33 33 33 33 M— 33 M0.094 33 M0.094 10 33 33 4 8 8 5 M M M M Kin Kin vdB vdB Kin Kin Kin Bd Kin E 4.00 1.56 1.56 1.00 0.40 0.094 0.094 0.83 6.25 0.59 0.094 0.094 284 M Mayall(1946) vdB vandenBergh(1969) vdB vandenBergh(1969) Sb Strffmberg(1925) SI Slipher(1924) (b) RevisiontoHumason'svelocitybasedonsameplate. (b) (a) 198lApJS ... 45. .259W Ao 97 NGC 4372 M Mayall(1946) References: NGC 4147 References: Ao Mz V-28 NGC 3201 Ga Gamalej(1948) BS Burbidge&Sandage(1958) Pal 4^(UrsaMajor) References: V 65=HV10331 Mz V-30 Remark: HSt Hartwick&Sargent(1978) Reference: Pal 3(Continued) SW II-4ZNG1 SW 1-5Ga(11) Int BS 133 G Primary IDAltAveRefWtSpVB-VU-BRemarks SW Sandage&Walker(1955) © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Alcaino (1976) Geyer (1975) Kin 1 V 65 Kin 1 Kin 2 Kin 3 + 56 + 68.2 +163 +149 +184 +200 +232 + 83 +481 +503 + 41 +168 +487 +491 +505 +500.7 +114 +496 +491 +490 + 11 + 13 + 4 + 4 0: 18 18 13 33 33 33 33 57 2.3 9 4 7 2.8 5 7 5 6 6 6 6 Kin 1.23 M M vdB M M HSt Kin Kin Kin Kin Kin Kin Kin Kin G 4.00 2.04 2.78 2.78 2.78 6.25 5.62 1.48 0.094 0.094 2.30 0.59 0.094 0.094 0.031 3.83 285 A5: vdB vandenBergh(1969) Z Zinn(1974) ZNG Zinn,Newell&Gibson(1972) Mz HSt Kin Hartwick &Sargent(1978) Menzies (1967) Kinman (1959) 12.46 +1.67 14.44 +0.63+0.02SW 13.19 +0.95+0.65SW 17.92 +1.36 13.54V +0.49+0.26G0.5:fid* 11.79 +1.60 11.74 +1.45 Ao Mz =Ao157 Mz =Ao158 BS fid fid, =Ga(12) 198lApJS ... 45. .259W NGC 4372(Continued) Ao 141 Ao Ao 152 Primary IDAlt3DAveRefWtSpVB-VU-BRemarks References: NGC 4590(M68) Mz A100 V 27 Mz D24Kin2 NGC 4833 References: Remarks: Mz D75Kin1 V 2=HV3693 GBP Int Kin References: Remarks: NGC 5024(M53) F Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Alcaino (1974) =CoD -259367 Greenstein, Bidelman&Popper(1947) Kinman (1959) Feast (1966) Kin 2 Kin 3 V 27 V 2 Kin 3 + 61 + 69 + 90 + 88e +185 +200.9 +199 +208 +219 +225.8 +205 -109 -108 -140 -109 - 56 - 61e -165 - 83 -175 - 66 - 87 -200 -170 + 11 + 11 + 11 + 5 + 10 + 20 + 10 + 10 + 10 + 10 ap z 17 apz 15 11 14 33 33 33 33 17 19 12 45 19 37 33 33 52 37 3 5.1 9 6 9.1 Kin 0.51 Kin 0.75 M M M M Kin 4.63 LE GBP Kin Kin Kin Kin Kin M M M E SI Sf Sll 1.23 2.78 0.69 0.28 0.094 0.094 0.094 1.76 0.094 0.88 0.31 0.094 0.094 0.037 286 M4e M4 Me Kin Mz LE GBP LE 12.96+1.85+1.89Mzfid Kinman (1959) Mayall (1946) Menzies (1972) Lloyd Evans(1977a) 12.93 +1.65 13.01 +1.58 12.50 +1.59Mz 12.45 +1.61 Ao Ao Mz 0.76 fid,=FIHya* 0.84 fid,=RZMus* (c) (b) (a) 198lApJS ... 45. .259W ROA ROA M ROA ROA ROA NQC 5139(a)Cen) ROA ROA ROA ROA ROA ROA ROA 8Egl108 ROA C L Remarks: C S4R1-3ZNG13 E C References : C S4R2-30ZNG16 C S3R2-23ZNG7 C S1R2-21ZNG8 C L NQC 5024(Continued) Cl C S3R2-21ZNG2 C S4R2-1ZNG9 C S4R1-1ZNG1 C Q C F Primary IDAlt Int Ga 30 29 27 24 17 14 12 23 22 21 18 13 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem Mayall (1946) Edmondson (1935) Guffey (1966) Barnard (1931) =Ga 42 Cuffey (1965) Gamalej (1948) (c) WeightedmeanofvelocitiesduetoSlipher(revised), (b) RemeasurementofSlipher*splatebyEdmondson. (a) RevisionbySlipher,basedonsameplateasfirstentry. H 66632 Egl 120 Egl 104 A E Egl 101 Egl 40 Egl 103 ZNG 5 ZNG 10 ZNG 3 ZNG 11 G 398 G 77 Edmondson andSanford. + 32 + 52 +234 +243 +236.3 +220 +244 - 43 - 3 - 4 - 9 - 2 - 26 - 54 + 36 - 67 - 57 - 66 - 87 - 21 - 17 + 4 - 84 + 27 - 55 - 46 -108 - 87 - 84 - 15 - 30 + 4 + 4 + 4 + 4 + 4 Av 20 15 20 20 20 22 20 20 15 20 20 15 20 18 13 33 18 18 18 18 33 13 18 18 18 18 19 6 7 4.2 9 N H DP FD Ref 0.44 0.25 0.44 1.80 Wt 0.61 0.28 0.28 0.28 0.28 0.48 0.28 0.094 0.28 0.094 287 A0 III/IVHk A7 Ib A5 III/IV Kl (III) G8/K1 (III)Hk Sp Z Zinn(1974) C S4R1-1=Ga40’ ZNG Zinn,Newell&Gibson(1972) SI Slipher(1918) ZNG 5-Ga3 Sll Slipher(1919b) Sf Sanford(1919) Ref Hk Hk FD 10.70 10.84 10.85 10.97: +1.23: 10.80 10.72: +0.07: 10.38 10.51 10.39 10.07 10.66 +1.33 10.25 14.38 14.36 14.53 14.28 14.94 13.02 14.54 14.95 14.46 14.31 9.55 +0.42 +0.25 +0.36 +1.23 +1.10 +0.45 +1.30 +1.11 +1.19 +1.05 +0.76 +1.07 +0.93 +0.87 +0.86 +0.76 +1.01 +0.50 +0.04 +0.40 B-V +0.02 +0.33 CSb +0.79 DS +1.46 +1.12 +1.37 +1.09 G +0.79 DS -0.01 U-B RefRemarks H ROA ROA ROA Cl C C C Cl C Cl C C C G G G G G 1 1 fld, -Baf -G 319* fld, -In36* fld, -In13* “B 12=Ga8 fld* fld, -GY* fld, -In21* fld, -Bae* fld* fld, =Gß* fid, -BaE* fld, =BaF* fid, 2obs.* =Ga 23 =Ga 40 2 obs.* fld* fid, »B1* fid, -Ga2 fid fid, =Ga(19) 198lApJS ... 45. .259W Primary IDAlt NQC 5139(Continued) ROA 35Kin2 ROA 41 ROA 31H66408 ROA 39 ROA 36AF ROA 40 ROA 63 ROA 58 ROA 55H111051 ROA 53V170 ROA 50 ROA 66 ROA 65Kin1 ROA 64 ROA 62H63033 ROA 57 ROA 67Kin3 ROA 91G299 ROA 75 ROA 73G210 ROA 70 ROA 78 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem +228 +205 +232 +235.72 - 83 +215 +210 +236 +223.0 +232 +230 +237 +218 +235.5 - 68 +215 +212 +216.7 +238 - 55 +255 +213 +209 +242 +219 +242 +171 +210 +238 +256 - 10 +269 +218 +251 +234 +251.7 +246 +250.4 + 12 +228 +250 +219 +226.3 +239 +251 +241.8 +235 +244 +244.6 - 12 - 33 +244 +238 +213.9 - 25 + 4 + 4 +215 + 4 + 4 +215 Av 43 15 10 26 15 19 15 43 11 20 20 13 14 15 10 10 12 12 10 25 22 12 15 15 13 10 12 15 13 10 13 10 16 12 4 4 7 7 8.6 0.49 9 5.8 7.1 4.9 2.5 7 3.4 9 9 5.4 4.4 6 2.6 H Ref Kin H LEI H H H1 H Kin H H N H H H N H1 H H H SmW D Kin Kin SmW 0.44 6.25 2.04 2.04 0.69 0.59 0.44 0.28 0.44 6.25 1.23 0.83 0.59 0.69 0.15 0.69 0.054 0.44 0.44 1.00 0.054 0.39 0.44 0.59 0.21 2.78 1.00 1.23 1.00 1.00 2.04 1.23 1.00 Wt 4 288 0.46 0.48 0.69 0.35 0.56 0.41 0.66 0.64 0.51 0.41 0.27 0.57 0.66 0.35 0.64 0.13 0.59 CH CH Sp Ref VB-VU-BRemarks Hl 11.46+1.68+1.30CSb D 11.58+1.82 <11.58> <+1.70><+l.73>CSb 11.37:v +1.52:ROA* 11.40: +1.36: 11.21 +1.64+1.81Eg2fld* 11.22 +0.49: 11.45 +0.46ROA 11.37 +1.50+1.41CSb 11.15: +1.40:ROA=Mt29a 11.63 +1.29:ROA 11.61 +1.42 11.61 +1.50+1.37Eg 11.64 +1.42+1.18CSb 11.70 +1.64+1.62Eg 11.64 +1.505+1.39Eg 11.53: +1.39:ROA 11.53: +1.37:ROA 11.50 +1.65+1.71CSb 11.50 +0.41ROA 11.81 +1.39+1.24CSb 11.53 +1.615+1.58Eg ROA H fld* ROA ROA =A G* fld* fld* 198lApJS ... 45. .259W NQC 5139(Continued) Primary IDAlt ROA 101 ROA 94 ROA 109G62 ROA 102G200 ROA 95Bah ROA 132 ROA 124G170 ROA 118AH ROA 113 ROA 96G242 ROA 128G46 ROA 156AI ROA 153 ROA 145G2 ROA 133 ROA 184 ROA 179 ROA 166 ROA 164 ROA 159G381 ROA 186 ROA 183G149 ROA 182 ROA 173 ROA 201 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem + 35 +227 +199 +222 +198 +210.3 +252 +256 +260.3 +216 +225 +220 +229 +216 +225.3 +243 + 22 +235 +265 +269 +205 +277 +207 +272 +222 +263 +213 +190 +133 +285 +264 +230 + 50 +256 + 5 +246 +218 +214 +236.8 +212 +248 +267 +248.7 +248 +270 +226 +251 + 54 - 39 +224 +233 +234 -252 + 4 + 4 + 4 + 4 +215 + 4 + 4 + 4 + 4 + 4 + 4 + 4 Av 10 22 26 20 13 10 11 21 25 12 20 10 20 31 13 11 28 15 12 12 28 15 11 12 16 28 11 13 13 14 13 12 18 8 7 9 7 7.8 8 7 9 6.9 3.6 8.3 9 8 9 9 8 8 7 9 7.0 H Ref LEI H H H H H LEI H LE H H LE N H LE H N LEI LEI SmW H H LEI LEI 0.15 0.59 0.69 2.04 2.04 1.00 1.00 1.00 0.44 1.56 0.16 0.59 0.83 0.69 2.04 1.23 1.23 0.23 0.69 0.39 0.59 2.04 1.23 1.56 1.56 1.23 1.23 1.23 Wt 0.16 0.48 0.63 0.27 0.35 0.38 0.47 0.32 0.18 0.30 0.51 0.21 0.48 0.38 289 K4 : MI K4: Sp Ref VB-VIf-BRemarks LE LE LE 12.10+1.61 11.80 +1.395+1.18Eg 11.74: +1.14:ROA 11.77 +1.62+1.61Eg=Mt162a 11.83 +1.38+1.25CSb 11.76 +0.39+0.07CSb 11.68 +1.46+1.33CSbmem 11.76 +1.48+1.40CSb 11.78 +1.40+1.145Eg 11.90 +0.65+0.14G 11.87 +1.28 11.74 +1.71+1.92:LEI 11.76 +1.10:+0.75:G 12.16: +1.00:+0.71:N 11.93 +1.55+1.84CSb 11.95 +1.35ROA 11.99 +0.57-0.00G 12.03 +1.72+2.05LEI 11.99 +1.27+1.03G 12.04 +1.53ROA 12.02 +0.65ROA 12.01 +1.32+1.04CSb 12.05 +0.28 12.04 +1.42 12.00 +1.73ROA ROA ROA ROA ROA f Id fld* fld fld* fld* fld fld fld 198lApJS ... 45. .259W NOG 5139(Continued) ROA 409 ROA 330Mt138a ROA 320 ROA 300 ROA 276 ROA 242 Primary IDAlt ROA 1627 ROA 1577 ROA 1404 ROA 1263 ROA 1108 ROA 1026 ROA 542 ROA 451 ROA 447 ROA 425 ROA 421 ROA 357 ROA 342 ROA 286 ROA 248 ROA 1590 ROA 1455 ROA 1432 ROA 1409 ROA 1403 ROA 1400 ROA 1272 ROA 1256 ROA 1155 ROA 1152 ROA 1031 ROA 524 ROA 513 ROA 492 ROA 338 ROA 231 ROA 1626 ROA 1595 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem G 222 G 388 G 378 G 61 G 366 G 7 G 79 + 28 + 5 + 38 + 85 +231 +291 +223 + 99 +201 - 44 +226 +183 +231 + 57 +274 +102 +220.4 + 64 +240 +228 +231 - 52 +230 +249 +261 +177 +227 +203 +214 +233 +253 +223 +226 +222 +249 +206 +208 +241 - 2 - 42 -141 -160 - 68 + 4 + 4 Av 20 20 20 20 50 50 50 34 21 28 21 21 21 50 20 28 21 28 20 21 28 20 50 20 18 28 21 28 21 20 16 18 50 50 21 11 21 12 8 8 8 8 6.7 N N N LE LE1 N N NB1 NB H H LE LE N LE Ref NB1 NB1 NE NB1 NB1 NB NB1 NB NB NB NB1 N LE1 NB NB LE1 LE1 LE N LE1 LE1 LE1 Rg Rg LE Fl 0.23 0.23 0.13 1.56 Wt 290 0.18 CN 0.18 0.17 0.18 0.17 0.17 0.17 0.18 0.18 wkGbd 0.21 0.18 0.21 0.038 0.53 K5-M0 0.48 0.17 0.37 0.48 0.17 0.17 0.48 M2 TiO: TiO Sp LE NB1 NBl Ref LE Fl LE 13.51 13.47 14.39 13.96 14.58 14.08 15.12 13.37 12.83 +0.63+0.14G 12.46 12.36 12.22 13.01 12.83 +0.82+0.27G 12.78 12.64 12.39 12.31 13.62 14.76 13.42 15.45 13.44 12.67 12.75V 12.33 12.19 13.98 14.77 14.17 12.92 +1.04-0.09CSb 12.74 +1.53 12.50 12.23: 14.79 14.82 12.54 12.89 12.84 +1.31ROA +1.74 +1.50 +0.75 +0.58 +1.25: +1.57 +1.63 +1.23: +0.97 +1.258 +0.32 +0.973 +0.93 +0.14 +1.16 +1.073 +0.22 +1.082 +0.22 +0.950 +1.74 +1.48 +0.69 +1.58 +1.52 +1.84: +0.35 +1.02 +0.913 +0.719 +1.127 +1.132 +1.00 +1.73 B-V +1.94: LEI +0.03 G +1.57 CSb +0.78! +1.29 +0.26 +0.15 +0.72 +0.21 +0.91 +1.97: LEI +0.32 N +0.49 +1.09 +0.79 -0.58 U-B RefRemarks NB ROA ROA NBl NBl NB ROO NB NBl NB NBl NB ROA ROA ROA ROA ROA NB NRS NB NB NB NBl ROA ROA ROA ROA Rg ROA G fld * fld * fld fld fld fld fld fld fld fld fld fld fld fld fld 198lApJS ... 45. .259W ROA 6747 ROA 6712 ROA 6686 ROA 6680 ROA 6642 ROA 6698 ROA 6595 ROA 6566 ROA 6389 ROA 6355 ROA 6234 ROA 6110 ROA 6139 ROA 6113 ROA 6088 ROA 5943 ROA 6107 ROA 5941 ROA 5931 ROA 5919 ROA 5783 ROA 5740 ROA 5736 ROA 5701 ROA 5556 ROA 5318 ROA 5006 ROA 3881 ROA 3639 ROA 2229 ROA 3867 ROA 3812 ROA 3596 ROA 2797 ROA 2403 NQC 5139(Continued) ROA 3642 ROA 1853 Primary IDAlt American Astronomical Society •Provided bythe NASAAstrophysics DataSystem Ba d G 259 G 321 G 250 Be L +222 +220.9 +214 +234 +247 +223 +224 + 58 - 18 + 70 +223.14 +141 +120 + 2 + 46 +192. +108 +224 +225 +168 +241 +222 + 96 +244 +220 +223 +200 +245 +225 +252 +170 +264 +198 +240 +240 +244 +181 +241 +227.1 +232 - 30 +231 - 86 Av 50 20 20 20 20 50 20 20 20 50 20 50 20 20 20 20 20 20 20 20 20 20 20 20 20 16 50 20 20 50 20 20 16 20 20 20 20 16 13 18 2.8 0.34 5.2 NB1 NB NB1 NB1 NB1 NB1 NB1 NB NB NB1 N NB1 NB1 NB1 NB NB1 NB NB1 NB1 NB1 NB1 N N NB1 N NB1 LE NB1 NB NB1 NB NB1 NB1 NB NB NB1 N NB1 N Ref Eg 0.040 0.25 0.040 0.25 0.25 0.040 Wt 291 0.18 0.65 0.18 0.69 0.18 0.18 0.18 0.18 0.18 0.18 0.18 0.18 0.18 0.32 0.18 0.18 0.18 0.18 0.18 0.58 0.18 0.18 0.21 wkGbd? CH wkGbd MO: CH Sp NB1 NB1 LE NB1 NB1 Ref 13.32 +1.05 13.68 +0.58 13.89 +0.728+0.17NB 13.63 13.83 +0.85 13.54 +0.94 14.94 +0.860+0.24NB 14.03 13.21 14.92 13.84 14.00 14.04 13.36 13.50 13.16 13.07 13.13 13.65 14.50 13.88 14.29 14.20 14.45 +0.906+0.28NB 13.84 13.84 13.54 14.37 13.95 +0.71ROA 13.04 +0.86+0.31G 13.68: 13.53 13.09 13.86 +0.88+0.52NB1 14.31 +0.24+0.08N 15.63 -0.01-0.47Rg 14.18 -0.05-0.57N +1.074 +0.92 +0.84 +1.06 +1.04 +1.00 +0.06 +0.930 +0.96 +0.901 +1.07 +0.97 +0.93 +0.88 +1.04 +0.997 +0.995 +1.23 +1.54 +0.24: +1.06 +1.10 -0.04 -0.14 B-V +0.63 +0.44 +0.15 +0.50 +0.57 +0.92 +0.38 +0.62 +0.32: +0.57 -0.86 U-B RefRemarks NB1 NB1 ROA ROA NB1 NB1 NB NB1 N NB ROA NB1 NB1 NB NB1 N ROA NB1 N NB1 NB NB1 ROA CSb CSb NB NB1 G fld fld fld mem fld fld mem fld fld? fld fld fld?* fld 198lApJS ... 45. .259W NGC 5139(Continued) Primary IDAlt © American Astronomical Society •Provided by theNASA Astrophysics DataSystem H 61952 LEI A271 Kin 4 LEI A343 H 66446 V 1 LEI B298 LE A648 LEI A636 V 2 V 6 V 65 V 53 V 42 V 17 V 78 +232 +218 +193 +158 +210 +249 +214 +190 +208.8 +239 +205 +198 +217 +200 +221 +220 +211 +221 +219 +212 +176 +194 +212 +218 +206 +216 +243e +247e +212 +215 +214 +212 +232e +257e + 28 +272e +226 +225 +220e +269e +256e +255e +253e +266.2 +225.75 +196 - 53e+10apz + 38.4 - 28.8 - 55 - 94 - 73 -130 -104 -127 - 93.4 -131 - 98 - 98 -135 - 3 + 4 + 4 + 4 + 12 + 24 + 3 - 1 + 30 + 11 + 19 - 18 - 18 - 17 + 20 - 0.1 + 28 + 29 - 2.1 - 2 + 6 + 15 Av r ap 13 ap ap 13 ap 15 ap pr P P P P P P P P P P 16 13 15 13 13 21 13 11 13 10 19 11 22 13 12 43 22 57 22 11 11 13 25 39 68 36 19 14 12 5 4 4 8 5 5 6 6 3 1.9 8 4 4 8 8 5 6 5 8 8 4.1 8 0.43 4 9 2.6 H Ref LEI LEI H Js LEI LEI Kin Js LE Js Js Js Js Js J Js Js Js Js Js Js Js Js Js Js Js DFE DFE DFE LLF F DFE DFE DFE DEE LLF LLF DFE DFE DFE LLF LLF LLF LLF DFE DFE DFE LLF LLF GV GV GV GV 11.1 0.63 4.00 0.83 4.00 4.00 6.25 6.25 2.78 1.56 2.78 6.25 0.27 0.56 0.50 0.80 1.56 0.031 0.21 0.50 0.39 1.07 0.28 0.054 0.066 0.022 0.51 0.16 2.97 1.07 0.69 1.01 ,00 ,78 ,25 .00 ,56 ,56 Wt 0.25 0.32 0.27 0.59 0.32 0.32 0.17 0.67 0.33 0.69 0.36 292 CH Fl II FI lb F0 lb A8 II F6 Me FO II Fl II F2 II £M4 M4-5e M4:e FO lb F5 II F2 II M4-5e M4 :e Fl II FO lb FO II FO II ~KO M3-4 M4-5e FI lb FO lb FO II Ml :e M2:e FO II M2.5e M2e A4-A6 Fpc A5-A6 A4 A4-A5 Sp Ref Js Js Js Js J Js Js Js Js Js Js Bo Js Js Js Js Js Js Js Js DFE DFE DFE DFE DFE DFE DFE F DFE DFE DFE DFE DFE GV GV GV GV <10.85> <+0.68><+0.35>Js=HV224* <13.05> <12.68> <+l.76> <12.26> <12.5:> <+1.64:> <14.82> <11.98> 13.25 LEI 13.09 LEImem? 11.41: +1.72:H 12.54 LEI 11.66: +1.19:H 12.16 +1.50+1.10Bo 13.69 LEI 14.12v +0.24+0.19LLF <+1.59> <+1.35:> <+1.72> <+1.86>Eg <+0.17> <+0.38>GV B-V U-B RefRemarks ROA 0.85fid,=HV225 DFE =HV229 DFE DFE 0.138 0.40 0.254 0.560 0.478 0.199 0.684 0.615 0.547 0.410 0.342 0.581 0.997 0.900 0.790 0.640 0.935 0.811 0.765 0.33 0.08 0.30 0.73 0.08 0.04 0.12 0.73 0.16 0.65-1.81 0.12 0.46 0.42 0.39 0.13 0.057 0.00 0.68-1.60 0.20 0.14 0.47 0.403 0.35 0.08 0.04 0.44 mem, =HV265* =HV 240 =HV 276 fid, =HV301* fid, =HV288* 198lApJS ... 45. .259W NQC 5139(Continued) Primary IDAltvAveRefWtSpVB-VU-BRemarks ROA ROA ROA ROA ROA Remarks : References: ROA ROA ROA ROA ROA ROA ROA ROA Eg Eggen(1972) A Arp(1958) ROA ROA ROA ROA ROA ROA DP Dickens&Powell(1973) D Dickens(1972) Be Beiserene(1959) ROA 109 ROA DS Dickens&Saunders(1965) DFE Dickens,Feast&Lloyd Evans(1972) CSb Cannon&Stobie(1973) Bo Bond(1975) Ba Bailey(1902) j; 23 21 70 57 50 39 31 29 27 24 22 18 66 53 36 13 17 12 14 8 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem 1 =CPD -47°6032=CoD-47°8335 =CPD -47°6030=CoD-47°8332 =Ba d=Be8709-982=HD116615=CPD-46°6338 =CPD -46°6335 “HD 116602=CPD-46°6334=CoD-46°8632 =HD 116450=CPD-46°6328=CoD-46°8618 =HD 116993=CPD-46°6363=CoD-46°8664 «CoD -46°8670 =CPD -47°8347 »CPD -47°6026=CoD-47°8325 Variable. (Dickens,FeastandLloydEvans1972). =CPD -46°6353 =G 262=CPD-46°6358=CoD-46°8657.Possiblyvariable. =HD 116745=CPD-46°6345=CoD-46°8644 =CPD -46°6361=CoD-46°866l =Be 8752-458 -Be 8470-874 =Be 8746-931 =CPD -46°6360=CoD-46°8659 =CPD -47°6013=CoD-47°8306 =CoD -47°8302 V 152 V 129 V 164 V 162 =CoD -46°8635 Available photometry(Woolley1966,Eggen Geyer 1967)showslargescatter. + 36 +184 - 83 - 59 - 58 - 54 +212 +226 +181 +196.5 - 26 - 35 +202 - 27 - 45 -134 - 98 - 45 -132 - 69 - 68 - 39 - 22 41 30 38 37 49 42 12 16 30 35 10 1 1 r P pr P P P P P P pr pr P pr P 45 23 36 11 24 39 26 11 26 30 31 25 13 11 71 11 26 18 26 11 4 6.2 6 LLF LLF LLF LLF LLF LLF LLF LLF LLF LLF LLF LLF DFE DFE DFE DFE DFE DFE DFE DFE GV 0.077 0.72 0.17 0.066 0.15 0.15 0.11 0.049 0.16 0.54 0.76 0.15 0.79 0.15 0.070 2.97 0.10 1.86 0.37 0.36 293 M5 M4 M5(4?) A5-A6 -G8 ~G2 H Harding(1965) Eg2 Eggen(1961a) ROA 166PhotoelectricphotometrybyLloydEvans(1977ab) ROA 156=Be8676-515 ROA 145=Be8508-129 ROA 113=CoD-46°86l9 V 78=V814Cen V 65=V813Cen V 42Epochofmaximum:JD2441109:(afterDickens, V 1Adoptedephemeris:Max=JD2415030.1+29.34891E ROA 1256Velocitiesquotedfor1256,1403,and1853 ROA 330,357,421,425,447,451,513(seeremark, ROA 320Variable(Dickens,FeastandLloydEvans1972) ROA 182,201,231,248,276,286,300(seeremark, Hk Houk(1978) Hl Harding(1962) FI Feast(1973) F Feast(1965) ROA 3642=Be8247-119 ROA 3639=Be8195-123 ROA 2229=Be8566-815 ROA 1853(seeremarks,1256,1403) ROA 1403PhotometrybyEggen.(seealsoremark,1256) FD Fehrenbach&Duflot(1962) Egl Eggen(Woolley1966) G Geyer(1967) GV Geyer&Vogt(1978) DFE <11.74><+l.61><+l.55>Eg DFE DFE DFE DFE <12.19><+l.73><+1.89>Eg DFE GV <13.01> <11.3:> <+l.8:> ROA 166) ROA 166) average, atV. Feast, andLloydEvans1972). are themeanforthreestars. is systematicallyfainterby0.27mag, (Jones 1968). DFE DFE 0.96 0.83 0.67 0.87 0.79 0.50 0.966 0.84 0.81 0.73 0.62 0.48 0.90 fid, =HV352 198lApJS ... 45. .259W vZ 291 vZ 287 vZ 265 vZ 238 vZ 205 vZ 164 vZ 309 vZ 297 vZ 281 vZ 263 vZ 250 vZ 192 vZ 115 NGC 5272 Mt Martin(1938) LE LloydEvans(1977a) vZ 318 vZ 237 vZ 177 LLF Lichten,Liller&Freeman(1979) LEI LloydEvans(1977b) NGC 5139(Continued) vZ 194 Kin Kinman(1959) J Joy(1949) Js Jones(1968) Primary IDAltAveRefWtSpVB-VU-BRemarks 7 stars Int In Innés(1923) American Astronomical Society •Provided bythe NASAAstrophysics DataSystem (M 3) V 95 V 138 KU 88 JS AH JS U JS S ZNG 6 JS AE Zh 216 Sg III-63 Sg IV-25 Sg III-64 Sg IV-101 Sg III-28 Sg IV-27 Sgl X23 + 2.51 + 1.70 + 0.56 + 1.71 + 4.66-146.90r + 3.12 + 5.69 + 1.98 - 3.93 - 4.04-146.90r1.45GG -144.00 -163 -156 -149.70 - 2.17 - 2.13 - 2.13 - 2.05 -149.32 - 6.59 - 2.23 -150.9 - 1.01 - 0.57 -145.55 -157 -135 -156 -300e - 6.70 - 2.79 - 29 - 0.17 -163 -144 -121 -125 -142 -149.99 -190 -150 -180 -177 -168 + 4 + 5 -146.90 r -146.90 r - 0 -151.48 pr -4 p -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r 23 44 23 13 18 18 19 12 19 10 33 33 19 33 33 37 1.15 8 1.17 1.07 1.6 1.02 1.06 0.29 0.79 0.75 0.79 0.37 0.94 0.85 0.71 0.94 0.87 GG 0.86 0.82 0.88 0.32 0.80 0.84 0.77 0.84 0.74 0.83 M M M M M M GG Co GG 145 GG GG GG GG GG 169 GG GG GG GG GG 183 J J GG 135 GG 149 GG 89 GG GG GG 113 J GG 156 P J E Sf2 Sfl SI 113 24.9 25.3 1.56 0.19 0.63 0.32 0.19 2.20 2.14 2.17 2.16 2.10 2.17 2.15 2.17 2.19 2.08 1.00 2.20 2.15 2.14 2.17 2.17 2.18 0.094 0.28 0.75 0.094 0.094 0.28 0.094 294 Ml M2 KO lb M2e Kl G8 lb Rg Rodgers(1972) NB Norris&Bessell(1975) ROA Woolley(1966) N Norris(1974) NRS Newell,Rodgers&Searle(1969) NB1 Norris&Bessell(1977) SmW Smith&Wing(1973) <12.36> <+1.64> <12,36> -+1.51>Rv 13.74 +1.08+0.90JS 14.11 +0.95+0.69JS 13.16 +1.27 12.89 +1.42+1.40Sgl 14.37 +0.79Sg 13.80 +1.13Zh 13.26 +1.30+1.19JS 13.53 +1.11+0.90JS 14.09 +0.65+0.10Sgl 12.81 +1.37+1.26Sgl 13.85 +0.98+0.61JS 13.26 +1.29+1.16Sgl 13.99 +1.00+0.75JS 13.60 +1.13+0.87JS 13.77 +1.19Zh Rv Sg 0.23 0.02 0.4: 0.3: 0.16 0.15 0.00 0.26 (a) =Ga (.7) 4 obs. =Ba d* =JS AA* =Kti 22* =Zh 222 =B 7* =KU 78* =KU 69* =Ba e* =Zh 99 =B 9* =KU 15* =Kli 12* =Kli 2* =Zh 125 =B 11* fid, =Kli49* 198lApJS ... 45. .259W vZ 610 vZ 592 vZ 591 vZ 585 vZ 589 vZ 555 vZ 576 vZ 574 vZ 549 vZ 545 vZ 528 vZ 509 vZ 508 vZ 463 vZ 490 vZ 420 vZ 417 vZ 387 vZ 398 vZ 334 NGC 5272(Continued) Primary 3DAltvAveRefWtSpVB-VU-BRemarks r © American Astronomical Society •Provided by theNASA Astrophysics DataSystem V 153 KU 348 KU 331 B 52 B 53 B 50 V 219 B 49 B 47 B 46 B 45 V 210 B 44 B 41 B 39 B 32 Sg III-80 B 30 Sg III-77 Sg IV-17 + 2.77-146.90r + 1.71 - 0.79 - 1.43 - 3.91 - 7.35 - 4.46 - 4.97 - 3.43 -150.02 - 3.50 - 6.33 - 0.41-146.90r - 5.10 -151.92 - 4.01-146.90r -143.11 - 9.21 + 8.07 + 6.79 -152.91 + 5.17 + 7.26-146.90r + 8.74 - 10.41 + 1.10-146.90r -156.60 - 6.77-146.90r - 1.69 - 5.46 - 1.34 -148.34 - 4.20 - 4.85-146.90r -151.54 -140.28 -146 - 6.94 -163 -139.38 - 4.36-146.90r - 5.89 -162 -166 -173 - 3.03 -161 -155 -153 - 5.52 -176 -156 - 7.97 - 6.68 4.47 3.32 -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r + 4 -146.90 r -146.90 r + 5 + 5 + 1 -146.90 r + 4 -146.90 r -146.90 r -146.90 r - 3 -145. -143. - 0 - 1 -144. -143. - 5 -142. - 5 -141, 13 pr 70 pr 58 pr 76 pr 92 pr 91 pr P P P P P P P P P P 18 13 13 23 23 18 13 18 23 23 1.00 1.23 0.90 GG 0*85 1.16 1.03 GG 0.81 0.95 0.83 0.81 1.05 1.27 1.25 GG 0.70 0.72 0.94 0.74 0.06 0.95 GG 0.88 0.99 0.82 0.56 1.23 GG 0.59 0.91 1.08 GG 1.19 GG 1.45 0.58 0.16 0.53 1.32 GG 0.73 0.60 0.86 GG 0.71 GG198 1.71 0.92 GG118 0.94 0.86 GG- 0.65 0.84 0.68 0.85 0.88 GG 138 GG 145 GG 66.1 GG GG GG 193 GG GG 204 GG 183 GG GG 102 GG 149 GG GG 129 GG GG 297 GG 121 188 356 142 237 138 129 216 74.3 90.7 62.0 34.2 0.33 0.33 0.32 0.63 0.19 0.19 0.63 0.19 0.63 0.32 0.19 0.32 2.16 2.17 2.15 2.17 2.16 2.16 2.15 295 2.20 2.16 2.19 2.18 2.20 2.10 0.14 2.18 2.17 2.13 2.16 2.12 2.17 Ml Ml G5 lb F8-G0p Kl G8 G5e G8e G4e G5e G8e G5e P P J J J J J J J J J J 12.91 +1.33Sg=KU325* 12.84 +1.42Khl=KU308* 12.59 +1.54 12.70 12.68 13.28 +1.17Khl=Khtt 12.58 +1.55 13.30 +1.15+1.16 13.28 +1.13 13.40 +0.39 13.85 +0.99 13.27 +1.20 13.26 +1.29 13.57 +1.19 Khl =KU300* Khl =KU192* Zh =KU293* Zh =KU287* Khl =KU278* Sg =KU247* JS =B31* Sg =B36* SD =B33* SD =KU166* Sg =B15* 0.98 0.90 0.84 0.88 0.85 0.83 0.77 0.72 0.68 0.67 0.65 0.52 0.50 0.35 0.34 0.31 p=Ga 23? =KU 330* =B 51* =KU 316 =B 42* =KU 262 198lApJS ... 45. .259W vZ 622B56 vZ 618B55 NGC 5272(Continued) Primary IDAltAveRefWt vZ 670 vZ 612B54 vZ 682 vZ 647B58 vZ 640JSA vZ 729 vZ 726 vZ 684 vZ 706 vZ 673B61 vZ 763 vZ 752 vZ 748 vZ 746 vZ 733 vZ 688 vZ 672B62 vZ 716 vZ 790B88 vZ 764B82 vZ 803V154 vZ 796B90 vZ 779B86 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem B 67 B 64 B 60 B 65 B 75 B 71 B 69 B 79 B 77 B 74 B 73 B 81 B 78 + 1.84 + 3.72 + 0.99 + 10.41 + 11.30 + 0.16 +146.35 + 0.15 + 6.29 + 3.43 + 0.04 + 1.59 + 3.49 -143.18 +15.95 -146.90r + 18.17-146.90r + 17.17-146.90r + 17.17-146.90r + 16.81-146.90r -140 + 3.01-146.90r0.85GG + 5.34 -158.72 - 9.22 + 2.28-146.90r1.04GG -136.01 - 2.96 + 3.22-155.11pr1.10GG 82.6 - 5.11 - 4.89 - 11.00 - 12.41 ^ 4.31-146.90r0.79GG - 6.17 - 2.72 -129.93 - 3.34-: - 4.94 -140 -142.72 - 3.29 -151.28 -150.09 -163 -173 -180 -165 -150 - 4. -180 -174 3.89 -146.90r 09 -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r + 14 + 11 -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r + 9 + 12 + 16 + 14 -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -5 p -145.07 pr •146.90 r ■146.90 r 22 22 13 13 13 13 13 13 15 1.04 1.01 1.00 0.05 1.11 GG81.2 1.01 0.70 0.85 0.92 0.71 1.13 GG78.3 0.96 0.84 0.71 0.82 0.77 0.41 0.78 0.44 0.64 0.84 0.77 0.80 0.74 GG 0.77 0.74 0.63 0.69 GG210 0.31 0.76 0.96 0.66 0.84 0.92 0.90 GG123 0.77 GG169 0.74 0.53 0. 90 GG GG GG 198 GG 142 GG 198 GG 138 GG 164 GG GG GG GG GG GG 149 Sf GG GG 169 GG 169 GG GG GG GG GG GG 98. GG 109 GG 183 GG J1 J1 J1 J1 J1 J1 J1 Sf 0. 123 0.052 0.63 0.63 0.63 0.63 0.63 0.63 0.44 052 2 2.20 2.15 2.15 2.18 2.19 2.16 2.16 2.18 2.19 2.17 2.17 2.17 2.17 2.18 2.18 2.18 2.15 2.17 2.17 2.16 2.18 2.15 2.19 296 KO IbP12.78+1.42Sg=KÜ352* G5 lb F8 F6 F8 F6 F5 G8-K0 IbP12.62+1.50Sg F8 GO Sp RefVB-VU-BRemarks P J1 J1 J1 J1 J1 J1 J1 <12.32> <+0.47> 13.31 +1.26Sg=B57* 13.65 +1.14Khl=KU359* 12.86 Zh=KU358* 13.56 1.05Sg 12.90 +1.20SD 0.51 0.48 0.33 0.08 0.41 0.29 0.18 0.09 0.05 =Kü 395b =KU 378 =KU 396 =Kü 417 =KU 413* =Kü 412 =KÜ 401 =KL CS* =Kü 469* =KU 451* =KÜ 442* =KU 488 =KU 479 =KU 470* =Kü 459 =Kü 456 =KÜ 433* =Kü 468* =B 91* =KÜ 482 198lApJS ... 45. .259W vZ 853 vZ 837 vZ 835 vZ 849 NGC 5272(Continued) vZ 1008 vZ 893 vZ 887 vZ 885 vZ 874 vZ 860 vZ 859 vZ 858 vZ 855 vZ 1059 vZ 1000 vZ 976 vZ 972 vZ 964 vZ 925 vZ 917 vZ 911 vZ 898 vZ 871 vZ 807 vZ 1053 Primary IDAlt vZ 928 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem V 225 B 96 B 92 B 109 B 106 B 105 B 103 B 102 B 98 B 126 B 107 B 104 B 130 B 125 B 124 B 117 B 113 B 112 B 131 B 127 B 123 B 121 B 120 B 115 Sg V-41 Sg V-80 + 14.82 + 7.35 + 2.22 + 7.87 + 10.65 + 1.53 + 6.63 + 4.32 + 10.53 + 9.74 + 4.97-146.90r + 1.59 + 7.71-146.90r + 3.03 + 3.85 + 3.95-146.90r + 0.46 + 2.53 -134 -141 -128 -121 - 0.82 - 3.75 -158 + 7.77 + 8.41 - 22.24 - 1.71 -148.18 -151.3 -194e -137 + 5.93 - 24.14 - 23.03 -136.91 -167 - 2.09-146.90r -139 -135 - 22.71 -169.79 - 0.66 - 0.33 -144.90 -139.25 - 3.20-146.90r - 6.61 - 1.31 - 5.56 -140.11 - 4.44 + 7p -146.90 r -146.90 r -146.90 r -12 p - 16p -163.04 pr -146.90 r -146.90 r - 0p - 4p -5 p - 16p -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -162.00 pr - 16p -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r Av 10 10 13 13 15 13 23 15 1.16 1.07 1.06 1.11 1.51 1.30 1.05 1.03 1.11 1.09 1.48 8 3.3 2.5 1.46 1.32 1.11 1.02 1.06 0.79 0.69 0.99 0.96 GG 0.80 0.52 0.78 0.71 0.37 0.30 0.74 GG 0.84 0.71 0.26 0.77 GG 0.77 0.72 0.92 0.77 0.84 0.37 0.67 0.54 0.75 0.73 GG 0.75 GG GG Jl Jl Jl Jl J1 GG Ref GG GG GG GG GG GG 81.2 GG 43.9 GG 59.2 GG 223 GG GG GG 178 GG Co 1. GG 142 GG 198 Jl Jl Jl GG Jl GG 169 GG GG GG 74.3 GG GG GG 81. GG 84, GG 45. GG 33. GG 156 GG 193 GG 46. 57. 0. 0. 0. 0. 0. 0. 0. 0. 44 44 4 19 95 63 95 9 63 63 Wt 1.77 2.18 2.18 2.20 2.15 2.20 2.16 2.15 2.15 2.17 2.14 2.18 2.15 2.16 2.19 2.17 2.15 2.15 2.15 2.18 2.19 2.17 2.17 2.17 2.19 297 G8 lb F6e GOe G2e G2e G3e G2e Gle GOe G5 lb Sp Ref Jl Jl Jl Jl Jl Jl Jl Jl P 12.70+1.50 <12.72> <+1.45> 13.79 +0.88+0.55JS 12.92 +1.42 13.01 +1.40 12.95 +1.36 13.50 +1.07 13.55 +1.19 B-V U-B RefRemarks Rv Khl Khl Zh Sg SD Sg 0.87 0.92 0.80 0.72 0.71 0.70 0.1: 0.99 0.89 0.87 0.74 0.65 3 obs. mem, =K(1581 =KU 563 =Kü 532* =KU 674* =KU 616 =Kü 609* =Kü 592* =KU 546 =KU 543 =KU 545* =Sg 11-46* =KU 669 =KU 634 =KU 629 =KÜ 586* =Ku 576 =B 110* =KU 550* =KU 544 =KU 540 =KU 570 =KU 552 =B 99* (a) - 1981ApJS... 45. .259W NGC 5272(Continued) vZ 1127B136 vZ 1082B132 vZ 1128Sg11-57-156.42 vZ 1121B135 vZ 1100 Primary IDAlt vZ 1203 vZ 1142 vZ 1135 vZ 1274 vZ 1219 vZ 1214 vZ 1208 vZ 1273 vZ 1224 vZ 1217 vZ 1376 vZ 1362 vZ 1360 vZ 1345 vZ 1270 vZ 1397 vZ 1383 vZ 1241 vZ 1449 vZ 1402 vZ 1392 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem B 134 B 137 B 138 KU 947 JS BC B 145 B 140 JS BI JS BF Sg 1-108 Sg 1-76 KU 950 JS AV Sg 1-109 Sg 1-106 Sg 1-46 Sg 1-92 Sg 1-87 Sg 11-18 Sg 1-81 Ga (25) Sg 1-21 + 3.04-146.90r + 1.61 + 1.45 + 2.09 + 1.24 + 2.88 + 9.26 + 5.66 + 0.64 + 3.19 + 0.59 + 3.70 + 11.85 - 11.57 + 0.19 + 1.51 - 1.12 -144.81 - 8.81 -157.72 -145.36 + 3 + 1.44 - 1.91 - 1.81 -153 -140 - 11.80 + 1.07 -145.41 -140 -148.02 - 11.12 - 10.61 -157.75 -157 -157 - 4.99 - 5.95 -146.63 - 2.78 - 0.07 - 3.00 -147.2 - 3.38 -162 - 2.04 - 2.42 - 2.49 -149.89 -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r -146.90 r Av 13 15 22 22 1.51 1.00 1.34 1.01 1.24 0.10 1.06 1.70 1.39 1.13 0.93 GG 0.82 0.89 0.92 0.93 0.08 1.2 1.62 1.55 7 0.95 0.97 0.18 0.66 0.87 0.81 0.25 0.03 0.69 0.87 0.93 0.33 0.65 0.89 0.96 0.86 0.89 0.97 0.92 0.89 0.83 0.55 0.62 0.77 0.24 8 Ref GG 112 GG Hb 2. GG 111 GG 149 GG 126 GG GG GG 132 GG GG 116 GG GG 152 GG GG GG GG GG GG GG 106 GG 126 GG GG GG GG GG 106 SSRI 0. Sf2 0. GG SS 0. GG 118 Co GG 331 GG 260 Sf2 0. GG 169 GG — GG 237 GG 145 43. 55. 1.56 052 052 Wt 2 2.20 2.20 G8lb 2.16 2.16 2.15 2.20 2.15 09V 2.18 2.18 2.13 2.20 2.11 2.14 2.20 2.20 2.08 2.16 2.15 2.17 2.16 2.07 2.09 2.17 2.13 2.20 — GOV 298 K0: lb G8 lb Sp Ref VB-VU-BRemarks P 12.97+1.23 SSRI 14.94-0.30-1.11Sgl 14.21 13.30 +1.26 13.29 +1.24 13.62 14.01 13.82 14.69 13.86 12.88 +1.18 13.17 +1.26 12.66 +0.64+0.09Sgl 12.65 +1.56+1.63Sgl 14.11 13.84 13.54 14.09 13.70 14.30 +1.05 13.37 +1.27 12.78 +1.41SD 13.05 12.88 +1.48 12.94 +1.22 +1.04 +1.37 +1.03 +1.16 +1.04 +1.06 +1.05 +0.75 +1,32 +1.11 +0.94 +0.49 Sgl +0.58 JS +0.75 JS +0.63 JS +0.74 JS +0.79 JS +1.10 JS Khi =Kü708* Khl Zh =KU694* Khl Sg Sg Sg Sg SD Sg SD Sg Sg Sg =ZNG 1* =KU 724* =B 143* =KU 798* =B 139* =Kü 744 =Kii 729* =KU 935 =KU 917* =Kü 846* =B 147* =Kü 852* =B 142* =B 141* =Zh 655 =KU 944* =Kii 928* =KU 820* =B 144* =Kü 737* 3 obs. =KU 916* =Kü 908* fid, =Zh657 198lApJS ... 45. .259W vZ 555 vZ 509 vZ 706 vZ 684 vZ 640 vZ 612 vZ 591 vZ 585 vZ 545 vZ 528 vZ 463 vZ 417 vZ 265 vZ 263 References: vZ 622 vZ 618 vZ 589 vZ 576 vZ 549 vZ 420 vZ 398 vZ 309 vZ 291 vZ 281 A Arp(1955a) vZ 490 vZ 387 vZ 318 vZ 192 vZ 334 vZ 250 vZ 238 vZ 237 vZ 205 vZ 194 Remarks: Co Cohen(1978) Ba Bailey(1902) B Barnard(1931) vZ 177 vZ 115 NGC 5272(Continued) Primary IDAltvAveRefWtSpVB-VU-BRemarks Hb Herbig(Whitford1960) Gr Greenstein(1935) Ga Gamalej(1948) GG Gunn&Griffin(1979) E Edmondson(1935) J Joy(1949) 7 stars Int r © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Mean ofvelocitiesduetoSlipher(1918),Sanford(1919a), =Zh 379.Sanford(1919a)listsonlythemeanvelocities -Zh 394 -Ga 42 »KU 375»Zh382 =Zh 375=Ga47=Khß =Zh 373=Ga7 »Zh 361=Ga43 =Zh 362=Ga46 =Kh y =Kh ç =Zh 356=Ga8 =KU 264=KhX29.Suspectedvariable(Kholopov1963). =Zh 335 =KU 227 »KU 197=Zh307=KhX8.Suspectedvariable(Kholopov =Zh 288 =Zh 211 *=Zh 206 “KU 56=Zh192 =KU 326=Ga1?Notvariable. =Zh 353 =Zh 349=Ga45=Kha =Zh 302=Ga21=Kh6 =KU 175=Zh294 =KU 119=Zh248 =KU 107=Zh235=HV850.Epochofmaximum:JD2427249.5 =Kil 101=Zh229 =B 3=KU67=Zh203 =B 1=KU50=Zh184 =Zh 136=0b325 -Kil 84=Zh217 =Zh 182 =Zh 157=0b328 =Zh 150 =Zh 148 =Ga (31) Sanford doesnotidentifythesestars,butheisknownto (a) SpectrogrambySanford. of vZ612,752,1127and1208,quotedhere close visualcompanions(Kii196,198). and Edmondson^remeasurementofSlipher’splate. and 1208(Sanford1919a,ShapleyDavis1920,Joy have obtainedspectraofvZ318,612,752,982,1127 individually foreachofthesestars. 1963). Spectraltypeaffectedbycontaminationfrom 1949). (Greenstein 1935). 299 vZ 1383-Zh646 vZ 1362-Zh629 vZ 1273-KU844-Zh562 vZ 1270-Zh559 vZ 1217-KU805-Zh526-Ga28 vZ 1208-Zh519.(seeremark,612). vZ 1203-KU792-Zh515 vZ 1135-Zh485-Kha vZ 1082-Zh469 vZ 871=Zh427-Khe vZ 835=Zh420=Khd vZ 803=KU514.Adoptedephemeris:Max=JD2438873.53 M Mayall(1946) vZ 1392-Zh653 vZ 1376-Zh641 vZ 1345-Zh616 vZ 1274-Zh564 vZ 1241-Zh542 vZ 1224-KU808-Zh530 vZ 1219-KU806-Zh527-Ga15 vZ 1214-KU803-Zh525 vZ 1128-KU728-Zh478 vZ 1127-Zh479-Ga4.(seeremark,612). vZ 1121-Zh476-Ga40-Khb vZ 1059-Ga14 vZ 1000-Zh442 vZ 972-Ga5 vZ 925=Zh433 vZ 917-Ga25-KhX20.Suspectedvariable(Kholopov1963). vZ 885=KU564 vZ 855-Ga12 vZ 853-KU541=Zh424 vZ 837=B97=KU534-Zh419 vZ 796ThisstarismisidentifiedasB92inKlemola vZ 752=Zh402-Ga2.(seeremark,612). vZ 748»KhX18.Suspectedvariable(Kholopov1963). vZ 746-Ga11 vZ 726-Ga31 vZ 716-Zh397 vZ 1360-Zh626 vZ 1100-Zh472-Ga39-Khc Rv Russev(1971) Kh Kholopov(1963) KU KUstner(1922) K1 Klemola(1979) Khl Kholopov(1977) P Popper(1947) Ob Osborn(1973) JS Johnson&Sandage(1956) J1 Joy(1940) (a) Meanof7plates. + 15.28539E,afterGreenstein(1935)and Hogg (1973).Thisstariserroneously identified asvZ801inSawyer(1955). (1979). 198lApJS ... 45. .259W NGC 5272(Continued) Primary IDAltvAveRefWtSpVB-VU-BRemarks Reference: NGC 5286 NGC 5466 Hop 15 Hop 36a Hop 30 Kin Hop 165 Hop 155 Int Hop 132 Hop 60 Hop 43 Sf2 Sanford(1919a) Hop 206 SD Shapley&Davis(1920) SI Slipher(1918) Sfl Sanford(1918) Sf Sanford(1919b) Hop 216 Hop 179 Sy Sawyer(1955) Sgl Sandage(1970) Sg Sandage(1953) r Hop 237 References: Remarks: Hop 216 Hop C Bd © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Kinman (1959) »BL Boo.ConsideredbyHogg(1973)afieldstar,this Hopmann (1922) Cuffey (1961a) Baade (1926) C B C F C S3RL C A V 19 C P C S3R1' C G C S1R2' C Y C 0 C S4R2-22+123.9 C N+47 variable isamemberaccordingtoitsradial velocity, colors,andluminosityclass. -10 +125 ■18 +102 ■15 +113 + 35 + 38 + 61 + 45 + 79 + 18 + 6 +101 +106 + 75 +103 +115.3 +118 +104 +120 +124 + 92 + 92 +120 +117 +137 +166 +117 +117 -110 +124 +128 + 5 + 5 + 5 + 5 16 18 18 18 28 18 18 18 18 18 18 11 17 12 10 15 12 14 18 18 Í7 13 16 16 7 7 5 7 6.6 6 3.2 6 Kin Kin Kin Kin ZD ZD ZD ZD ZD ZD ZD ZD ZD ZD ZD ZD ZD ZD Z 0.35 0.26 0.30 0.24 0.23 0.32 0.30 0.45 0.21 0.42 0.10 0.35 0.45 0.39 0.59 4.00 0.39 2.04 2.04 0.30 0.30 0.30 0.30 0.30 0.30 2.05 6.37 300 A2-F0 V vZ vonZeipel(1908) W Wallerstein(1958a) SSRI Strom,Rood&Iben(1970) ZNG Zinn,Newell&Gibson(1972) Zh Zhukov(1971) Z Zinn(1974) SS Strom&(1970) Z Zinn(1974) ZNG Zinn,Newell&Gibson (1972) ZD Zinn&Dahn(1976) (b) SpectrogrambyKraft. (a) ThevelocityquotedbyZinn(1974)isameanofthese ZD three plates. <14.75> <4O.20><+0.12>ZD 14.19 14.11 13.63 14.38 14.10 14.05 14.00 14.43 13.56 14.21 13.60 13.57 +0.72 +0.53 +0.36 +1.11 +1.37 40.84 +1.35 +0.55 +1.18 +0.89 +0.41 +1.28 0.764 0.513 (b) 0.331 0.302 0.124 (a) 0.086 0.970 0.893 (a) 0.868 0.513 (a) 0.188 0.536 man?, =ZNG3 =Bd r =ZNG 6 =C L* fid, =ZNG2 fid, =ZNG1 fid, -ZNG4 fid 2 obs. 198lApJS ... 45. .259W KU 186V42 KU 108AIII-3 NGC 5904(M5) M Mayall(1946) Reference: NGC 5824 M Mayall(1946) References: Int NGC 5694 HaH Harris&Besser(1976) Reference: NGC 5634 Int Primary IDAltAveRefWtSpVB=VU-BRemarks Int Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem + 44 + 45 + 53 + 48 + 46 + 67 + 42 + 47 + 64 + 35 + 36 + 42 + 56 + 80 + 52.70 + 45 + 3 + 74 + 68 + 42 + 56 + 30 + 10 + 49.7 + 89 + 74 + 68 - 6 -174 -161 -198 -188 -202 18 49 96 45 68 52 56 98 + 6 + 14 + 17 + 3 + 9 + 3 + 13 + 13 r 12vdB r 11vdB z 10Kin 13 13 13 13 13 12 SHS 16 Z 19 M 33 M 13 E 33 M 33 M 37 SI 33 M 33 33 33 33 28 33 33 33 33 33 33 33 33 4 4 4 4 4 4 4 4.3 W1 2.5 2.5 0.66 M M M M M M M M M M M HaH M 5.69 5.69 5.69 5.69 5.69 0.63 5.69 0.63 5.69 0.63 0.63 0.63 2.19 1.00 5.41 0.33 0.69 0.094 0.094 0.28 0.094 0.56 0.094 0.094 0.094 0.094 0.094 0.094 0.13 0.094 0.094 0.094 0.094 0.094 0.094 0.094 301 F5 F5 F8 F6 F8 F4 F6 M Mayall(1946) W W J <11.22> <+0.60><+0.36>A1=B18* 12.42 +1.49+1.59Eg=B4* 0.40 0.35 0.38 0.35 0.21 0.21 0.20 0.18 0.30 0.12 0.09 0.03 0.01 0.01 } (a) 3 obs.(a) (b) 198lApJS ... 45. .259W 53 NGC 5904(Continued) KU 756 Kli 753V50 KU 752B168 Primary IDAltAveRefWtSpVB-VU-BRemarks Remarks: KU 1007 KU 912 KU 752®Zh669=Ga25’.Spectrogram byWilson. KU 186Sw159=Zh347=HV534.Adoptedephemeris:Max= KU 108=Sw90=Zh280=Ob503 Int (a)CombinationofSlipher'sVelocitywithremeasurement © American Astronomical Society • (a) Linesaredoubledatthisphase;highervelocity (b) TheIndicationbyKinman(1959)thatthisisastellar V 84 A IV-59+58 A IV-27+58.1 velocity isatypographicalerror. by Edmondsonofthisandtwootherplates. components arelistedfirst. JD 2427567.8+25.7325E(Arp1955a). + 42 + 80 + 73 + 76 + 87 + 34 + 55.1 + 72 + 50.1 + 36 + 47 + 55 + 52 + 30 + 65 + 35 + 52.5 + 51 + 75 + + + + ' + + + + 86 + 75 + 70 + 56 + 67 + 29 + 45 + 48 + 47 + 49 + 55 + 61 + 47 + + + + 51.6 + 24 + 23 + , 33 46 69 59 61 52 51 78 34 70 38 37 52 59 63 65 61 + 4 + 4 + 9 + 23 + 25 + 11 + 14 + 17 + 5 + 2 + 14 + 13 + 10 - 2 + 28 + 25 + 13 - 24 - 25 - 19 - 2 - 10 - 2 + 31 + 31 - 17 - 16 - 3 - 4 - 24 - 24 - 8 - 24 - 19 - 13 - 10 - 1 - 2 - 15 - 25 - 27 - 25 - 14 - 8 18 18 13 13 18 13 13 18 13 13 23 23 18 13 13 13 16 Z 18 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 4 1.0 8.7 1.8 W1 2.5 4 4 4 4 2.5 1.9 W1 3.1 w w w w w W W w w w w w w w w w w w w J w J W W J W1 w J J J J J J 0.30 0.19 0.30 5.69 5.69 0.19 5.69 5.69 5.69 5.69 5.69 5.69 5.69 5.69 0.32 5.69 0.63 0.63 5.69 5.69 5.69 5.69 5.69 5.69 0.63 0.63 0.63 0.32 5.69 5.69 5.69 5.69 5.69 5.69 5.69 5.69 5.69 5.69 5.69 5.69 0.63 0.32 0.63 0.63 0.63 0.32 0.33 Provided bythe NASA Astrophysics Data System 2.06 2.16 0.83 2.04 0.33 302 Ml MO KO G3 G3 F5 G4 G2 GOe G2e G5 F7e F5 GO F5e G2 G5 KU 756=Sw729=Zh672=HV576.Adoptedephemeris: KU 1007=Sw950=Zh870=Ob559 KU 912=Zh786.SpectrogrambyDeutsch. KU 753=Sw727-Zh671=HV542 (a) SpectrogrambyDeutsch. <11.45> <+0.57><+0.31>Al 12.63 +1.34 15.18 +0.86 Max °JD2415027.5+53.283E,afterArp maximum followingthedeeperminimum corresponding to=0.0. and twomaximaoccurpercycle,withthe (1955a, 1957)andHogg(1973).Twominima ST ST 0.76 0.72 0.50 0.98 0.90 0.89 0.66 0.56 0.52 0.45 0.22 0.20 0.16 0.11 0.03 0.98 0.98 0.92 0.89 0.87 0.56 0.52 0.37 0.35 0.24 0.13 0.05 0.98 0.97 0.94 0.85 0.84 0.79 0.75 0.69 0.66 0.58 0.57 0.54 0.47 0.45 0.42 0.37 0.28 - (a) } (a) =B 171* =Sw 723* =B 225* =B 172* =Sw 857* 198lApJS ... 45. .259W NGC 6093(M80) HSt Hartwick&Sargent(1978) Reference: HSt 28+85 HSt 24+79 Reference: NGC 5986 Pal 14_(A-vdB) A& Andrews,Feast,LloydEvans,Thackeray&Menzies(1974)KinKinman(1959) V 3Adoptedephemeris:Max=JD2441507+310E(Andrews, F Feast(1973) References: V 3 Int Remark : M Maya11(1946) Int NGC 5927 A Arp(1955b) Ob Osborn(1973) Kü Küstner(1933) Ga Gamalej(1948) A1 Arp(1957) References: Kin Kinman(1959) NGC 5904(Continued) J Joy(1949) E Edmondson(1935) B Barnard(1931) Int Primary IDAltvAveRefWtSpVB-VU-BRemarks r © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Mayall (1946) et al.1974). + 45 + 43 + 70 + 9 +115 - 3 + 363 - 16 - 98 -64 -4p42 - 7118 -118 53 - 6834 -118 37 -204 90 23 40 37 33 33 28 33 33 33 33 M M E HSt HSt SI A& 0.055Me Kin 0.025 Kin 0.087 Kin 0.31 Kin 0.073 Kin 0.012 Kin 0.036 303 0.094 0.094 0.19 0.062 0.12 0.094 0.094 0.094 vdB vandenBergh(1969) Wl Wallerstein(1959) W Wallerstein(1958b) Z Zinn(1973) Zh Zhukov(1971) Sw Shilow(1898) ST Simoda&Tanikawa(1970) SHS Smith,Hesser&Shawl(1976) SI Slipher(1918) F 0.00 * 2 obs. 198lApJS ... 45. .259W V 6 NGC 6093(Continued Primary IDAlt V 1 V 7 Remark: Lee 3713Kin1 References: Lee 1412V4 NGC 6121(M4) Lee 2406V13 J Int Eg E Lee 4613Kin3 Lee 4611Kin2 Lee 1412=HV1114=CoD-26°11309 Remarks: Ao References: Lee 3713=Ao571 Lee 2406=HV1123=CoD-26°11313 Gr Egl Eg American Astronomical Society •Provided bythe NASAAstrophysics DataSystem Combination ofSlipher'svelocitywithmeasurementby Eggen (1961) Edmondson (1935) Joy (1949) Alcaino (1975a) Eggen (1972) Greenstein (1939) Eggen (1977) R Sco S Sco Edmondson ofsameplate + 15 + 8 + 12 + 6 + 4.2 + 21 + 68e + 78.2 + 85e + 95e + 78e + 57e - 5.3 - 14e + 55.1 + 22 + 77 + 80 + 75 - 15e + 73 + 58 + 94 - 2e - 10e + 77 + 69.4 + 57 43 52 53 61 69 + 5 - 15 + 0 + 0 Av ap ap ap ap ap ap 13 ap 13 ap 13 ap 18 16 18 18 18 18 23 33 18 13 33 15 13 13 18 18 13 12 13 13 23 5.5 2.2 6.1 4.5 4 7 5 6 6.5 Ref M M M Me Me Me Me Me Me Me Me Me Kin Kin Kin Kin 0.30 0.19 0.28 0.52 0.28 0.52 0.52 0.28 0.28 0.28 0.52 2.04 6.25 0.18 0.30 0.55 0.42 0.47 0.47 0.47 0.47 0.27 Wt 2.31 0.86 0.28 0.094 0.094 1.70 1.55 2.09 0.60 304 M(3)e M(3)e F6e GO KO G2 G6 G3 G8 G8 G4 G6 G3 Sp Me M Lee 4613=Ao516 Lee 4611=Ao515 Lee SI Kin J Ref Me Me Merrill (1941) Mayall (1946) Lee (1977a) Slipher (1922) Kinman (1959) Joy (1949) <13.64> <+0.77><+0.22>Eg <10.83> <+l.75><+1.83>Egl <10.6> <+1.61><+l.60>Egl 10.80 +1.93+2.04Eg 10.97 +1.965+2.23Eg 11.21 +1.71 B-V U-B RefRemarks Lee 0.29 0.96 0.10 0.07 0.03 0.78 0.93 0.04 0.03 0.16 0.03 =HV 585 =Gr 581* fid fid =Gr 363* =Gr 261* =Gr 259* =Gr 113* 198lApJS ... 45. .259W L 199 L 158 L 172 L 96 L 72 L 26 L 2 L 139 L 88 L 43 L 16 4 stars NOG 6205(M13) References: V 1 Remarks : V 1 Reference: NOC 6171 NOC 6139 DR Primary IDAltvAyeRefWtSpVB-VU-BRemarks D Kin Int Int Int r © American Astronomical Society •Provided by theNASA Astrophysics DataSystem V 720Oph>-50 Dickens (1970)andRolland(1972)relabel Kinman (1959) K 385 K 369 K 331 K 310 K 268 K 234 K 377 A 11-25 K 289 K 357 K 259 Dickens &Rolland(1972) V23 asVI. Dickens (1970) + 66 -260 -216 -258.1 -251 -213 -232 -226 -244 -255 - 10 + 1 -292 -257.3 -265 -265 -256 -209 -263 -242 -230 -239 -217 -244 -223 -217 -221 -200 + 19 -230 -240 -154 -300 -121 -120 -192 - 12 + 13 - 7 - 7 - 7 - 7 - 7 - 7 - 7 - 7 21 21 21 33 33 21 21 21 21 21 23 35 33 33 67 10 21 13 11 13 10 33 37 33 11 33 33 12 10 19 19 10 17 8.3 5 5 9.7 NZ NZ NZ NZ NZ M M M Co NZ NZ NZ vdB P M M M Mo M Co NZ E M M Kin M Kin Z Sb Kin Kin SI Kin DR Gr Gr 4.00 0.22 4.00 0.22 0.84 0.20 0.20 0.20 0.69 0.20 0.20 0.59 0.094 0.094 0.19 0.094 0.022 0.66 0.20 0.20 0.094 0.75 0.094 0.28 0.094 0.094 0.35 0.83 1.00 0.094 0.28 1.00 1.00 305 Me G5 lb G5-G8 lb G5 lb Mayall (1946) Feast (1972) 12.20 +1.39+1.22Ct 13.60 +0.99+0.66K 15.43 -0.17-0.60K 15.82 -0.08A 12.70 +1.19+0.95Ct 12.52 +1.27+1.09Ct 13.70 +0.94+0.39K 14.62 +0.85+0.37K 12.32 +1.30+1.16Ct 13.56 +1.00+0.62Ct 14.00 +0.75+0.24Ct -AJ J38* -A II1-63* -A 11-57* -A 11-76* 2 obs. -A II1-73* mem, 2obs.* -A 11-14* »Sr 59 =AJ J49* «AJ J50* -A III-45* fid, «DD27* (c) (a) (b) 198lApJS. L 487 L 598 L 530 L 526 L 469 L 403 L 326 L 267 L„ 324 L 306 L 222K393 NGC 6205(Continued) L 636 Primary IDAltv,AveRefWtSpVB-VU-BRemarks L 745 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem V 10 A 11-48 K 455 K 443 K 463 K 425 K 426 K 421 K 483 Sr 449 Sr 388 Sr 485 -276 -252.0 -249 -270 -259 -234 -252.0 -246.4 -246.0 -272 -257 -248 -241 -257 -248 -253 -249 -217 -263 -193 -245.0 -248.0 -263.0 -244 -243.2 -246 -251 -241 -234 -‘266 -239 -251 -248.7 -239 -225 -243.0 -254.0 -260.3 -239.3 -259.1 -237 -281 -252.8 -257 -235 -260 -290 -255.5 -242 -216 -244 -246 -251.8 -241.9 -244.5 -259.8 -259.1 -258.2 -256 -223 -252 -248 -245.4 + 3 + 17 - 11 - 12 - 6 - 19 - 6 - 7 - 12 - 20 13 18 13 10 18 13 18 10 13 13 13 18 18 18 15 13 18 18 18 23 21 21 23 13 18 13 13 23 13 13 18 21 18 23 13 13 4.6 1.6 4.3 1.8 1.0 8 4.3 5 2.1 4.4 8.7 4.6 4.4 8.0 8.3 1.4 2.4 7.9 9 2.5 5.9 9.0 6.1 9 7.9 9.6 6.8 Co 4.00 NZ NZ NZ SSRI Z 0.31 Z Z Z SGr 22.7 SGr 30.9 SSRI SGr SGr 100 SSRI 1.69 SSRI SGr SGr SGr SGr SGr SSRI SGr SGr SGr SGr SGr SGr SGr 17.4 4.73 1.32 1.60 1.12 1.12 1.60 2.87 1.09 1.56 1.45 5.17 2.16 0.63 0.31 0.18 0.19 0.32 0.19 0.63 0.63 0.31 0.56 0.93 0.63 0.32 0.63 0.45 0.45 0.45 0.27 0.45 0.45 0.54 0.27 0.29 0.29 0.54 0.29 0.29 0.18 0.29 1.77 1.91 1.15 0.38 0.62 0.77 A3III(?)SSRI13.79+0.23 0.20 0.20 1.89 1.40 0.20 0.56 1.46 306 KO (comp?)SSRI14.02+1.02 Br A5 lbSSRI13.92+0.44Br KO G5 KO J G3 FO B9-A0 V B5 V G8 J G8 J F5 F5 G2 G2 J G2 J G6 J G2 G5 G8 G8 F2 G2 GO GO G5 J G5 J G5 G5 SGr 12.03:+1.58:B SSRI 13.69+0.21 r <12.98> <+0.31> <11.83> <+1.62> 12.6 v+1.24Br 13.14 -0.16-0.80Sg 14.59 +0.78+0.27Ct 14.61 +0.85+0.40K 12.54 +1.28+1.14Ct 13.19 +1.05+0.82K De RR1 ^0.74 0.39 0.39 0.00 0.59 0.55 0.86 0.75 0.74 0.16 0.26 0.43 0.46 0.62 0.82 0.79 0,82 =B 161* =A 1-13* 3 obs. =B 123 =Sr 356* =A II-l* =ZNG 2* =A III-33* =A II-4* =Sv B651* =ZNG 4* =V 11* »B 140 2 obs. =V 2* 2 obs. 3 obs. 3 obs. Ha) Ha) Ha) ) (a) Ha) Ka) 198lApJS ... 45. .259W L 199-Sr130-Ox30-Bm5 L 172-Sr112=B17 L 158-Sr103-Ox26-Bm7 -Ga 45 L 139-Sr92-Ox25-SvB818 -Ob13818 L 96-Sr63-Ox22=B7-Bm6 L 72=Sr48-Ox18-SvC245 L 43-Sr29-Ox14-SvB273\ L 26-Sr14=0x11=B1»SvB286-Ga8 L 16=Sr8=SvA479 L 2“AJJ81=Sr»SvA233=ZNG7 4 starsMeasurementbyAdams,Joy,andHumason(Mayall1946). Remarks: Int (a)VelocityincludedinmeanquotedbyEdmondson(1935) L 1073 L 1043 L 1041 L 1023 L 1019 L 973 L 993 L 984 L 961 L 954 L 872 L 863 L 816 NGC 6205(Continued) Primary IDAlt American Astronomical Society •Provided bythe NASAAstrophysics DataSystem (c) (Seeremark,Int(b)). (b) MeasurementbyWright;thisplatewasremeasured K 699 K 656 K 422 K 286 K 228 K 224 K 210 K 188 K 604 K 577 K 567 K 566 Sr 776 K 544 K 553 K 548 V 6 K 538 K 536 K 500 Sr 660 Mayall (followingentry). Stars notidentified. -228 -259 -247 - 87 -235 -219 -229 -245 -204 -247 + 18 -248 -260 - 33.4 - 37 -249 -214 -213 -283 -230 -224 -263 -247.7 -237 -256 -244 -246 -249 -245 -253 -261 -227 - 7 - 7 - 7 - 7 - 7 - 7 - 7 - 7 - 7 - 37 - 7 + 14 - 7 - 7 - 7 + 2 - 17 + 30 - 31 - 7 Av ,21 21 21 , 21 18 21 21 21 29 21 10 21 18 10 21 21 17 21 23 23 15 13 15 21 13 12 9 7.2 9 5 5.8 5 . NZ NZ NZ NZ NZ Z NZ NZ NZ NZ W Gr NZ z NZ NZ NZ Z 0.93 Co SSRI 1.12 J J Co 4.00 NZ 0.22 Ref 0.31 1.23 0.18 0.18 0.35 0.63 0.36 Wt 0.20 0.20 0.20 0.20 0.20 0.20 0.11 0.20 0.20 0.66 307 0.20 0.20 0.28 0.20 0.20 1.33 1.18 0.48 0.50 F8 V A3-5 III-VSSRI14.02+0.09 KO lb F5 A8 F2 A2 F2 L 469 L 403 L 326 L 324 L 306 L 267 Sp L 222 Ref -Sr 288-Ox36-Ob13651 -Sr 345-SvB841-Ga50 -Sr 234-Ox34=B166=B -Sr 231=B64.Twomaximapercycle,interchang- -Sr 188=B157=B44 -Sr 216-Ox32-B162=B59-Ga21-HV588 -Sr 148-Ox31=B147=B29-ZNG1-KS9. (a) Theprecedingandfollowingvelocitiesof <12.04> <+1.49> <14,00> <+0.42> <14.00> <+0.20> 13.75 14.02 11.99 13.35 14.54 13.04 14.33 12.88 13.53 13.39 15.81 12.70 +0.67+0.15Ct 12.99 13.69 40.75 13.39 +0.91 12.09 +1.54 12.85 +1.15 + 1035N.Max-JD2438228.8591.77E measures ofthesameplatebyStoecklyand Greenstein, respectively. ing asprincipalmaximumatT=JD2436370 by Greenstein(1968). Greenstein (1968)werepreviouslysummarized Results ofthemeasurementsbyStoecklyand (Russev &Russeva1979b). this pairofentriesareindependent (N even);=JD2438272.44+91.77 (Nodd). 40.95 40.065Sgl +1.12 40.94K +0.97 +0.42K +1.09 +1.30K +1.05 40.73K +0.88 40.25K +0.88 +0.41Sgl +1.05 +0.68Sgl +1.01 +0.95K +0.81 +0.42K +1.12 -0.01 B-V +0.24 Ct +1.64 Ct U-B RefRemarks A K K RR K De A De 0.12 0.69 0.75 0.39 0.05 =AJ X24 =Sv A371* fid* =AJ J3* =AJ J37* =Sgl A10* =Sgl A1 =Sv B171* =Sv A317* =A 1-75 =A IV-61* =A IV-52* =A 1-54* fid* 3 obs. =A 1-48* 2 obs. =A 1-53* 4 obs.* =Sr 667* =A 1-42* =V 1* 198lApJS Primary IDAlt L 636Strom,etal.(1970)identifythisstaras656(=Sr501 L 487=B109 L 973=Sr831=B234=Bm3=KS34.Variablestar:Max=JD L 961=Sr731=0x50=B231 L 872=B1109=B216 L 745=Sr578=B184=SvC24 L 530=Sr394 NGC 6205(Continued) A Arp(1955b) Mo Moore(1932) De Demers(1971) AJ Arp&Johnson(1955) L 954=AIV-25=Sr726=Ox48=Bac=B229=Ga6 L 863=B215.ThisstarisidentifiedbyJoyas"thenearby L 816=Sr630=B1100=B202=Ga24=HV587 M Maya11(1946) References: Gr Greenstein(1968) NGC 6218(M12) K Kadla(1966) Ga Gamalej(1948) Ct Cathey(1974) Bf Brown(1955) Ba Bailey(1902) L Ludendorff(1905) E Edmondson(1935) Co Cohen(1978) Bm Baum(1954) B1 Barnard(1914) B Barnard(1931) KU 76 KS Kollnig-Schattschneider(1942) J Joy(1949) KU 190 KU 104 KU 99 4 stars KU 308 KU 307 Int KU 423 KU 413 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem Rc IV-1-24 Rc 1-1-2 Rc 1-1-1 Rc 1-1-16 Rc II-2-51 V 1 Rc II-2-47 =Sch 163c=ZNG6).Themarkeddiscrepancybetween actually thestarobserved(Cudworth1979a). 2441069.6 +43.04E(Russev&Russeva1979a). their spectraltypeandthecolorindexofL656 south precedingcompanionstar"toV6. (B-V =-0.27)leaveslittledoubtthatL636was +160 + 19 + 57 + 30 + 39 - 68 - 50 - 32 - 38 - 34 - 29 - 58 - 40 - 42.4 - 42 - 45 - 47 - 50 - 39 - 32 - 44 - 28 + 1 + 2 + 8 + 5 - 7 - 8 - 12 Av 33 33 33 33 22 22 21 23 12 23 13 11 10 13 13 13 13 16 16 13 6 5.1 Ref M M M M Ab GN GN GN GN GN GN HS J J J J J J J J Sf 0.63 0.62 0.62 0.62 0.19 0.19 0.60 Wt 0.22 0.72 0.85 0.20 0.69 0.38 0.37 0.54 2.28 1.74 308 G5 GO F8 F8 G2 GO cKO GO Sp L 1043=Sr778=Ox57=Bm13 RR Russev&Russeva(1979a) NZ Norris&Zinn(1977) K 224=SvA210=BrN7 L 1073=Sr799=Ox62=Bad=Ga5=0b13171 L 1023=Sr768=B244 L 1019=AIV-60=Sr766=B1133=B243 L 993=Sr749=0x53=B1124=B239=ZNG3 L 984=Sr745=B238 vdB vandenBergh(1969) K 286=AJX20=Bab=BrN13=SvA171=ZNG5 K 228=SvA522=BrN10 K 188=Ga(32) RR1 Russev&Russeva(1979b) P Popper(1947) Ob Osborn(1973) K 656=BrN21 K 210=BrN3 Ox Plummer(1905)COxfordU W Wallerstein(1958a) ZNG Zinn,Newell&Gibson(1972) SGr Stoeckly&Greenstein(1968) Sch Schlesinger(1934) Sb Strömberg(1925) SSRI Strom,Rood&Iben(1970) Sv Savedoff(1956) Sr Scheiner(1892) SI Slipher(1918) Sgl Sandage(1970) Z Zinn(1974) Sg Sandage(1969) Ref 12.96 +1.10 12.29 +1.36 13.18 +1.22 13.53 +1.09 12.83 40.98 12.52 +1.26 B-V U-B RefRemarks Rc Rc Rc Rc Rc Rc 0.86 0.80 0.62 0.39 0.34 0.27 0.15 -NH B862 -NH D5519 =NH C543 -NH B861 4 obs.* “NH C556 -NH D5520 (b) (a) 198lApJS ... 45. .259W NGC 6218(Continued) Remarks: Ab Abt(1955) References; Primary IDAlt3DAveRefWtSpVB-VU-BRemarks NGC 6229 HS Besser&Shawl(1977) 4 starsStarsidentifiedonlyas"fournearnucleus". KU Küstner(1933) M J Joy(1949) GN Gratton&Nesci(1978) Remarks; Int (a)RevisionbyMayall. NGC 6254(M10) References; A E Int A A Int A A A Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem 1-2 1-35 1-34 1-32 1-25 1-15 1-33 Mayall (1946) Edmondson (1935) Combination ofSlipher'svelocitywithremeasurement (b) Alternativevelocity+100±12km/spossible. V 2 B 22 HRR 480 ZNG 1 ZNG 4 ZNG 2 by Edmondson(1935). This isthebasisofclustervelocityquoted of sameplatebyEdmondson. + 26 + 71 +104 + 40 + 45 + 90 -144 -100 + 60.6 -210 -135 + 70 + 25 -122 + 67 + 57 + 94 + 78 + 38 -173 -149 + 55 + 51 + 80 + 15 +109 -166 + 64 + 36 + 13 + 13 + 24 + 33 - 12 - 26 - 3 - 38 - 25 12 19 23 33 33 52 33 33 13 13 23 14 13 13 13 13 13 13 33 25 26 33 33 33 27 13 5.7 8 9 M M M M M vdB M M M M E vdB E SI GN GN J J J J J J J GN GN SSRI SSRI SSRI 0.63 0.065 0.63 0.63 0.63 0.63 0.63 0.63 0.094 0.28 0.094 0.19 1.67 0.68 0.094 0.094 0.19 0.094 0.094 0.094 0.094 0.51 B3-5lb?SSRI13.23 -0.04 0.15 0.13 13.23 +1.13 309 AO IIISSRI13.51+0.15 F8e A7-FO IIISSRI13.97+0.54 F8e F5e GO G2 GO GOe M Mayall(1946) KÜ 308Joy(1949)identifiesthisstarasthefollow- Rc Racine(Alcaino1973) NH Nassau&Hynek(1942) vdB Sf Sanford(1919b) SI van denBergh(1969) Slipher (1922) <11.83> <+0.79> 13.07 +1.28 12.83 +1.27 with V1. ing andusuallyfainterofaclosepair A1 A A A HRR HRR HRR 0.44 0.88 0.61 0.53 0.03 0.82 0.08 mem?* mem?, 2obs. 3 obs. fid 198lApJS ... 45. .259W M M References: A A IV-44 A IV-15 A III-16 A 11-50 Kin Remarks: GN A1 References : A 1-35(seeremark,1-34) A III-21 A 11-72 A 11-24 A 1-60HRR466 E NGC 6266(M62) HRR Remarks : NGC 6254(Continued) J E B Primary IDAltAveRefWtSpVB-VU-BRemarks Int Int 1-34 © American Astronomical Society • (b) CombinationofSlipher'svelocity(astabulatedby (a) AccordingtoMayall(1946),thechangeofsignfrom Mayall (1946) Mayall (1946) Arp (1955b) V 1 Arp (1955a) Harris, Racine&deRoux(1976) Gratton &Nesci(1978) HRR 73 HRR 15 Kinman (1959) Edmondson (1935) Photometry givenforthisstarinTable2ofHarris, Ob 1018 B 8 Edmondson (1935) Joy (1949) Barnard (1931) B 23 B 2 ZNG 7 ZNG 3 B 1 Racine &deRoux(1976)actuallyreferstoHRR 480 =A1-35(Harris1980). velocities arebasedonthesameplate. Slipher’s velocityisatypographicalerror; + 35 + 50 + 86 + 78 + 80.8 + 70 + 53 + 29 + 12 + 73 + 73 + 83 + 56 - 61 - 64 -158 -134 - 63 - 45 - 2 - 88 - 50 - 35 - 19 - 27 + 1 10 19 33 33 33 37 37 33 23 17 37 18 16 13 12 18 18 10 14 23 17 13 13 3.8 9 M M M M M M Kin E W 1.23 GN GN GN 0.69 GN GN GN GN Sb SI Z Z Z1 0.29 0.53 Provided bythe NASA Astrophysics Data System 0.28 1.00 0.094 0.094 0.19 0.35 0.51 2.39 0.32 0.45 0.28 0.32 310 GO G4 GO V f vdB vandenBergh(1969) W Wallerstein(1958a) A IV-44=HRRC Ob Osborn(1973) Ob 1018PhotometrybyMcClure. Sb ZI Zinn(1973b) SI Z Zinn(1974) SSRI Strom,Rood&Iben(1970) ZNG Zinn,Newell&Gibson(1972) (c) CorrectionofEdmondsonsmeanbyMayall. Edmondson. Theerrorofsignispropagatedinto this weightedmean. Strömberg) withremeasurementofsameplateby 11.75 +1.17HRR 11.52 +1.20 11.85 +0.87 11.79 +1.58 11.94 +1.52 12.51 +1.49+1.42Ob 12.37 +1.35 12.10 +1.46 12.30 +1.47 12.97 +1.-29 Slipher (1922) Strömberg (1925) A A A A A HRR HRR HRR =B 15 * fid, =HRRD fid, 2obs.* fid fid (a) (c) (b) 198lApJS ... 45. .259W NGC 6333(M9) M Mayall(1946) Reference: NGC 6304 M Mayall(1946) Reference: NGC 6293 M Mayall(1946) Reference: M Mayall(1946) References: Int NGC 6284 Remarks: E Edmondson(1935) NGC 6273(M19) Int -102 Int Primary IDAltAveRefWtSpVB-VU-BRemarks Int Int (a)RemeasurementofSlipher'splatebyEdmondson. Int +30 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem +225 +237 +225 + 19 +116 + 51 + 34 +119 + 54 +140 +120 +153 + 71 - 50 + 50 - 15 -117 - 41 -107 - 82 -1^7 -115 - 54 + 13r14vdB 23 E0.19 33 M0.094 37 SI 33 M0.094 33 M0.094 33 M0.094 33 M0.094 33 M0.094 33 33 33 33 33 33 33 19 M 33 23 E 33 M 33 M 37 SI 33 M 33 M 37 M M M M M 311 0.094 0.094 0.094 0.094 0.094 0.094 0.094 0.094 0.19 0.094 0.50 0.094 0.094 0.094 0.073 (a) vdB vandenBergh(1969) SI Slipher(1922) (b) WeightedmeanofvelocitiesduetoSlipherand Edmondson. (b) 198lApJS ... 45. .259W Primary IDAlt Remark: NGC 6333(Continued) M Mayall(1946) NGC 6341(M92) References: Hop 26SWVII-5 Hop 17SWVII-1 E Edmondson(1935)SISlipher(1918) Int CombinationofSlipher’svelocityandremeasurementsame Hop 46SWV-2-10 Hop 29SWVI-6 Int -160 Hop 47SWVII-18-121.57 Hop 31SWVI-7 Hop 75 Hop 49 Hop 132 Hop 123 Hop 119 Hop 178SWIX-6 Hop 157 Hop 138 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem ZNG 1 SW VI-18 SW IX-2 SW VII-67 SW VIII-43 SW VIII-44 SW IX-5 plate byEdmondson. +221 +196 +244 + 2 -150 + 21 - 86 -114 - 78 -110 - 90 - 50 - 91 - 63 -118 -137 -158 -113 -119 -112 - 94 -117.0 - 27 - 73 -114 + 1 + 1.0 + 42 -138 -122.7 -140 -129 -119.2 -151 -109 -103 -156 -145 -106 -116 -122 -117 -103 -128 -123 - 4 Av 4 4 4 r r r r r r r 33 33 33 33 33 37 33 40 40 22 33 22 16 22 NZ 22 15 10 19 19 22 NZ 15 18 15 15 18 15 11 18 22 NZ 16 15 15 15 SS 15 SS 15 SS 15 13 Z 15 SS 15 SS 8.5 0.9 0.90 9 5 8 Z2 8.0 1.2 M M Ref M M M M M M M WC 123 NZ NZ NZ NZ NZ NZ Gr E GN 0.062 HSt 69.4 HSt 0.062 SI Co 4.00 Z 0.22 Z1 Z1 SS Z1 0.22 SS 0.20 0.44 0.20 0.67 0.22 0.22 0.22 0.44 0.44 0.20 0.22 0.20 1.78 Wt 0.094 0.094 0.094 0.38 0.094 0.094 0.094 0.28 0.28 0.094 0.31 0.18 0.40 0.40 0.18 1.00 0.40 1.58 312 wkGbd wkGbd F8-G0 V Sp Ref VB-VU-BRemarks NZ Ct Z1 14.58 +0.89+0.49SWfid,=Boh8 13.50 +1.05+0.95 13.58 +0.69+0.16Ctfid?=Boh14* 15.08 +0.6640.10Ctfid,»Bob11 14.06 +0.83+0.26 13.77 +0.86+0.29 12.19 +1.30+1.06 13.16 40.8440.35SWfid,=Boh13 14.68 +0.8240.24 13.09 +0.6040.05 14.62 +0.7540.12 13.14 +0.61+0.10 14.70 +0.72+0.11 Ct =Boh21* Ct »Bob63* Ct =Boh23* Ct =Bob66* Ct =Boh39* SW fid,«Bob22* SW »Bob83* SW fid,»Boh79* SW »Bob69* 2 obs.* 4 obs.,(b) 3 obs. fid, 2obs.* } (a) (c) (b) (a) (a) (b) (b) 198lApJS. Hop 663 Hop 382 Hop 344 Hop 187SWIV-2 NGC 6341(Continued) Primary IDAlt Hop 949SWX-4-50 Hop 923SWX-49-136.31 Hop 728 Hop 657 Hop 624 Hop 543 Hop 222 Hop 983SWIII-65-125.2 Hop 773 Hop 741 Hop 702 Hop 694 Hop 538 Hop 723 © American Astronomical Society •Provided by theNASA Astrophysics DataSystem B 43 B 39 B 85 B 74 B 62 B 61 B 54 B 88 B 82 B 75 SW IX-81 SW IX-10 SW III-81 SW IV-40 + 20 + 20.0 - 99 -128.2 -119.2 -123.4 -121.0 -128.2 -123.7 -130 -109 - 71 -113.1 -124.2 -123.8 -120.0 -119.2 -112.9 -117.5 -127.4 -115.6 -116.7 -118.2 -128.9 -128.49 -114.3 -116.44 -106 -118.9 -117.2 -112.6 -115.4 -113.3 -120.0 -117.6 -116.2 -121.5 -118.3 -113.7 -123.0 -120.4 -130.15 -118.9 -117.5 -114.7 -126.9 -130 -135.8 -141.5 -131.1 -129.7 -128.8 -116.2 -131 -124.3 -139 -135 -121 v JL 4 r22NZ Av eRefWtSpVB-VU-BRemarks 4 r30NZ 4 r22NZ 4 r22NZ 21 GN 15 SS 15 SS 15 SS 0.99 0.67 0.89 3.5 8.0 5 Co 2.0 WC 7 Z2 2.5 WC 3.3 2.0 WC 0.35 8 Z2 5 Co 2.0 WC 2.3 WC 2.6 WC 2.4 WC 3.4 WC 2.4 WC 2.7 WC 2.1 WC 2.3 WC 2.1 WC 2.1 WC 2.0 WC 2.2 WC 2.5 WC 2.0 2.2 WC 2.4 2.6 WC 2.2 WC 2.5 WC 2.1 WC 2.7 WC 2.2 WC 1.6 WC 1.8 WC 1.7 WC 1.6 WC 1.5 1.9 WC 1.9 WC 1.7 WC 1.9 WC 1.6 WC 1.3 WC 1.5 1.6 1.7 WC 1.6 WC 1.9 39.1 25.0 39.1 39.1 22.7 25.0 34.6 27.7 34.6 39.1 59.2 20.7 27.7 22.7 25.0 27.7 30.9 20.7 34.6 20.7 18.9 17.4 22.7 22.7 14.8 16.0 14.8 17.4 18.9 16.0 13.7 13.7 16.0 8.65 4.00 0.20 0.23 0.20 4.00 1.78 0.18 wkGbd 0.40 wkGbd 0.40 wkGbd 1.58 1.55 1.59 1.47 1.60 1.51 1.52 1.58 1.37 1.54 1.55 1.51 313 K2-5 V NZ Ct Z1 Z1 13.58 40.9140.45 12.86 +1.16+1.09Ct fid, 5obs.* 12.22 +1.2840.84Eg=B103* 12.92 +0.83+0.62 14.64 +0.74+0.19 13.94 +0.80+0.28 12.49 +1.19+0.81Ct =B 108* 14.37 +0.65+0.01Ct“B81* Ct mem,=»B6* Ct =Boh112* SW fid,=B21* SW =Boh131* «Sz 26* 3 obs. =Sz 21 =Sz 19* =Ga 3 2 obs. 4 obs.,(b) } (a) Î (a) }* }* >* }* }* }* >* }* }* }* }* }* } (a) }* }* (a) 198lApJS. NGC 6341(Continued) Hop 1046 Hop 1018SWXI-50+32 Hop 1130SWIII-13-112.96 Hop 1123SWXII-34-112.6 Hop 1100 Hop 1085 Hop 1028 Hop 1214SWXII-2 Hop 1211SWXII-1 Hop 1143 Hop 1131SWIII-12 Hop 1126SW11-39-77 Hop 1107 Primary IDAlt Hop 1219SWII-6-130 Hop 1213SWXI-4 Hop 1179SWXII-8-118 Hop 1176SWXI-3-79 Hop 1134 Hop 1215SW1-2-150 Hop 1210SWII-2 Remarks: Hop 31 Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem f Combination ofSliphersvelocityandmeasurementby =ZNG 4.SandageandWalker(1966) suspectthisstar (a) Remeasurementofplatetaken byStromand(1970). SW XII-45-122 SW SW III-ll-100 SW III-27-104 SW SW III-4 SW 11-89-104 Edmondson ofthisplateandoneother. of variability. XI-2 -80 11-24 -124 + 20 + 15 -107 - 98 -117.5 -112.6 - 97 -148 -102 - 92 -108 -127 - 31 -101 -130 -115 -108 -117 -111.6 - 92 - 62 - 90 -118 -128 -138 -163 -142 - 67 -146 - 29 - 78 -113.9 - 4 - 4 - 4 - 4 - 4 - 4 - 4 - 4 Av 15 45 15 15 15 15 10 15 18 15 11 15 15 40 11 15 15 26 20 15 13 20 15 10 20 20 22 15 31 15 22 20 52 20 22 22 22 30 12 1.6 1.0 1.1 0.87 1.5 2.5 5 Ref WC 82.6 NZ NZ NZ GN NZ NZ NZ WC 16.0 WC 39.1 Gr NZ NZ NZ Gr NZ Co — HSt 44.4 HSt 0.062 Z1 Z Z1 Z1 0.89 Z1 Z1 SS Z1 Z1 Z1 SS SS SS SS SS SS 0.44 SS 0.44 0.44 0.44 0.44 0.20 0.44 0.25 0.44 0.44 0.20 0.44 0.20 0.20 0.44 0.20 0.44 0.20 0.20 Wt 0.79 0.40 0.40 1.58 1.58 0.14 0.40 0.45 0.79 0.52 0.40 314 wkGbd wkGbd wkGbd wkGbd Sp Hop 46=Ga(37) Ref NZ Z1 Z1 Z1 (c) Meanofthreeplatespreceding. (b) RemeasurementofplatetakenbyZinn(see 15.23 +0.69+0.07SW 14.44 +0.88+0.55SW 13.45 +0.89+0.39Ct 16.15 -0.12-0.39SW 15.14 +0.75+0.08Ct 15.11 +0.82+0.37SW 14.28 +0.72+0.12Ct 14.38 +0.82+0.33Ct 14.08 +0.76+0.32SW 14.18 +0.73+0.13Ct 14.03 +0.78+0.21Ct 15.11 +0.18+0.08SW 14.66 +0.58+0.03Ct 12.76 +1.06+0.57Eg 13.55 +0.89+0.45Ct 14.26 +0.73+0.25SW 14.54 +0.78+0.16SW 12.19 +1.37+1.22Eg 12.89 +0.67+0.09SW 13.29 +0.76+0.47SW remark (c)). B-V U-B RefRemarks =Boh 280 =B 118* =Boh 267* “Boh 346 =Boh 329* =Boh 306* =B 116* =Boh 289 =B 111* =Boh 340 fid* =Boh 303* fid* fid?* fid* 2 obs. fid* fid* 2 obs. fid* fid* (a) (a) (a) (a) 198lApJS ... 45. .259W M Mayall(1946) NGC 6341(Continued) ABS Arp,Baum&Sandage(1953) References: Hop 178=PKh177V-67 V 3 NGC 6356 HSt Hartwick&Sargent(1978) GN Gratton&Nesci(1978) Gr Greenstein(1968) Ga Gamalej(1948) Hop 382=Nad=ZNG2=PKh155V-26 Hop 187=Boh100=0b9202 Hop 157=ZNG3 Hop 119“PKh176=PKhV-64 Primary IDAlt Hop Hopmann(1930) E Edmondson(1935) Ct Cathey(1974) Boh Bohlin(1906) Hop 344=PKh130IV-59 Hop 138=B2=Boh74=Sz3=Naa Hop 123“PKh163=PKhV-41 Hop 75=Na15=PKh202VI-41 Hop 49»PKh210=PKhVI-55 Hop 47=ABS1“Ob9218.Possiblyvariable(Arp,Baumand Eg Eggen(1972) Co Cohen(1979) B Barnard(1931) Hop 222=PKh274VIII-51 Int American Astronomical Society •Provided bythe NASAAstrophysics DataSystem (b) Meanoffourplates,includingonebyStromandStrom. (b) MeasurementbyGunnandGriffin. (a) Thesetwovelocitiesareevidentlybasedonthesame (a) (seeremark.Hop157(a)). (b) Meanoffourplates,includingonebyStromandStrom. (a) Zinn(1973b)suggeststhatvelocitieslistedbyStrom velocities forIX-5andIX-81.Thesearetwoof have herebeendiscardedonthestrengthofZinn's which areingoodagreementwiththoselistedby assertion thathisownmeasurementsoftheirplates and previousvalues,thethirdcasebeingXI-2(Hop and 1131),whichwererecordedonthesameplate. are infactmeasuresforXII-2andIII-12(Hop1412 half weightassignedtoeachentry. he findsverydifferentvelocities.Curiously,how- and Strom(1971)forIX-5IX-81(Hop157382) plate. Theoriginofthedifferenceisunknown; Sandage 1953;NorrisandZinn1977). identifications amongthesestarsremains. support hissuggestionthatanerrorofidentifica- stantial discrepanciesexistbetweentheirvelocities tion hasoccurred,butthepossibilityofothermis- three casescitedbyNorrisandZinninwhichsub- supported bylatervelocitiesobtainedNorrisand ever, hisvelocitiesforXII-2andIII-12arenot Zinn obtainsvelocitiesfortheselattertwostars 1143). TheoriginalmeasurementsofStromand Zinn (1977),which,however,agreewellwithhis Strom andfortheformertwostars,which + 23e + 2 + 31 + 19 + 12 + 78 + 7 + 13 Av 33 33 33 33 33 14 Ref vdB M M M M Wt 0.085 Me 0.094 0.094 0.50 0.094 0.094 315 Sp Hop 543,624,657,663,694,702,723(seeremark.538 Hop 538=Ga19 Hop 1018 Hop 983 Hop 949 Hop 923 Hop 773=Ga10 Hop 741(seeremark.538(a)). Hop 728»Boh186»Ob9281»PKh261=PKhVIII-31 NZ Norris&Zinn(1977) Hop 1131 Hop 1130 Hop 1126 Hop 1107 Hop 1046 Hop 1028 Na Nassau(1938) Hop 1214 Hop 1213 Hop 1210 Hop 1179 Hop 1176 Hop 1123 WC Wilson&Coffeen(1954) PKh Paneva&Khejlo(1966) Hop 1143 Hop 1134 Hop 1215 Ob Osborn(1973) ZI Zinn(1973a) ZNG Zinn,Newell&Gibson(1972) Z2 Zinn(1973b) Z Zinn(1974) Sz Schultz(1886) SW Sandage&Walker(1966) SS Strom&(1971) SI Slipher(1918) Ref »Boh 227»PKh136IV-69.Meanoffiveplates, =Boh 284=PKh73III-23 “Boh 259»PKh25=PKh1-29 »Boh 254=PKh78“PKhIII-32 “Boh 246=Sz34=Nac=ABS3=PKha =Boh 221-Sz29“Nab =Boh 304 “Ob 92013 »Boh 299“Sz37=PKh72III-22 =PKh 33“PKh1-45 =Boh 309=PKh134IV-66 =Boh 300»ABS11=PKhb29“PKh1-35 =Boh 342 =Boh 341 =0b 9208-PKh91“PKhIII-51 =PKh 371-53 “Boh 344 “Boh 343 “Boh 326“PKh88»PKhI11-47 (a) Theprecedingandfollowingvelocitiesofthis (a) (seeremark,Hop538(a)). (a) MeasurementbyGunnandGriffin. (a) (seeremark.Hop157(a)). (a) (seeremark.Hop157(a)). (a) (seeremark.Hop157(a)). pair areindependentmeasurementsfromthe same platebyWilsonandCoffeen,respectively. including threebyStromandStrom. (a)). B-V U-B RefRemarks 198lApJS ... 45. .259W V 3SpectraltypeduetoLloydEvans NGC 6356(Continued) Ao 17 Ao 14 NGC 6362 M Mayall(1946) Remark: Primary IDAltvAveRefWtSpVB-VU-BRemarks Ao 19 References: Ao 34 V 4 V 1 NGC 6388 Ao References: F Feast(1972)vdBvandenBergh(1969) A& References: Fc ROB 43Ao206 ROB 28 ROB 5 ROB 4 NGC 6397 F Int r Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Alcaino (1970) Fourcade (1974) Andrews, Feast,LloydEvans,Thackeray&Menzies(1974) Feast (1972) Kin 1 Kin 3 Kin 2 Kin 4 V 1 + 84 + 81 + 77 + 85 + 85 + 62e+7 + 76 + 76 + 84 - 9 + 41 + 6 - 25 - 23 - 15 - 24 + 18.2 + 26 + 22 - 11 - 7.3 + 18.28 - 29 " 23.3 - 39e - 22e 0 + 9 + 9 + 9 + 9 + 9 + 9 + 5 + 7 + 11 + 5 ap ap 11 12 14 12 15 15 15 16 33 24 30 6.8 4.4 4 7 5 9 6 7 5 3 3 7 7 0.7 0.77 A& Kin 0.83 Kin 2.04 Kin Kin Ma Ma Kin DC& 204 Ma Kin Kin Kin Kin Kin Kin Kin F F F Kin SHS SHS SR 0.39 0.39 0.27 2.04 4.00 316 11.1 11.1 1.93 0.085 Me 1.03 1.03 0.096 2.84 4.00 2.04 2.04 0.51 5.12 0.39 0.69 6.25 0.61 0.17 Me AO p Kin Kin SHS SR 13.43+0.18+0.20NRS KInman (1959) KInman (1959) Smith, Besser&Shawl(1976) <13.4> <+1.7><+0.53>ROB 11.81 +0.94+0.40Cn 12.77 +1.65 10.94 +1.12+0.74Cn 12.49 +1.64 12.54 +1.49 12.71 +1.60 Ao Ao Ao Ao 0.85 0.27 =Fc D =Fc G =Fc B =Fc C =SG 10-13* fld* 2 obs. 198lApJS ... 45. .259W ROB 48 ROB 44Ao212 ROB 75 ROB 74 ROB 70 NGC 6397(Continued) ROB 162 ROB 123 ROB 99 ROB 208 Primary IDAlt ROB 226 ROB 221 ROB 211 ROB 291 ROB 283 ROB 251 ROB 544 ROB 447 ROB 436 ROB 387 ROB 602 ROB 584 ROB 469 ROB 468 ROB 459 ROB 428 ROB 318 ROB 661 ROB 632 ROB 627 ROB 603 ROB 531 ROB 644 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem Ao 217 Ao 254 Ao 366 Ao 269 Ao 375 Ao 258 CS A14 Ao 275 CS A6 Ao D Ao 331 Ao E Ao 343 CS A19 CS 3 Ao 108 Ao 48 Kin 1 Kin 3 Ao B Ao 127 Ao 332 Ao 144 Kin 2 Kin 4 Ao 116 CS A8 CS A5 CS A15 CS A12 SG 16-10 + 6 + 17 + 17 + 40 + 14.4 + 9 + 30 + 29 + 29.60 + 22 + 11 + 10 + 21.1 + 7 + 12.4 - 41 .+ 9 + 39 + 23.5 + 19.0 + 4 + 21.07 + 5 + 5 + 35 + 23.99 + 3 + 19.7 + 22.5 - 11 - 14 - 61 - 15 + 23.7 + 27 - 8 - 3.8 + 16 + 17 - 63 - 3 + 28 - 22 - 1 - 17 - 7 + 5 + 5 + 5 + 5 + 5 Av 49 34 34 34 24 20 59 49 27 12 11 15 10 10 24 11 10 34 10 34 18 24 59 59 59 8 0.49 0.3 8 8 0.1 4 1.8 0.4 0.51 0.94 1.2 6 5 6.3 7 0.4 DC& 6 6 2.4 2.5 Ma Ma DC& Ma Ref Ma Ma Ma CS CS Ma Ma Ma DC& Ma DC& Kin Kin 2.78 DC& DC& 625 DC& 16.0 Kin Kin Kin 0.83 Kin CS SR CS Kin Kin 4.00 CS SR SR SR CS CS SR SR SR SR 0.17 0.25 0.14 1.00 1.56 1.56 0.086 6.25 Wt 0.085 A2p 1.21 0.085 AOp 0.029 AO 0.041 A1 0.041 A2 5.26 1.47 5.24 4.91 0.71 0.029 A1 0.61 1.70 4.51 0.085 AOp 0.029 AO 5.21 0.30 0.029 5.28 5.05 317 GO V sdOp Gp A2 FO III Kl IV/V F8 III F5/6 V B9p Sp CS CS Ref CS CS SR SR SR CS SR HC CS HC CS SR SR SR 12.44 +0.67+0.17Cn 10.74 +1.26+0.80ROB 13.27 +0.18+0.21NRS 13.24 -0.21-0.90ROB 13.33 +0.10+0.17ROB 13.00 +0.26+0.32Cn 13.08 40.21+0.21NRS 12.12 +0.87+0.29Cn 13.60 +0.15+0.07NP.S 11.21 +1.12+0.55ROB 10.59 +1.16+0.82ROB 10.78 +1.02+0.68Cn 10.16 +1.46+1.30Cn 12.73 13.14 10.76 +1.12+0.74ROB 11.18 +1.02+0.72ROB 11.03 +1.20+0.68ROB 12.64 13.58 11.50 11.16 11.24 11.50 10.97 13.22 13.33 +0.14+0.19Cn 13.00 +0.29+0.30Cn 10.35 9.98 9.42 +0.87+0.56Cn *.46 +0.53+0.10Cn +0.14 +0.15 +1.04 +1.33 +0.60 +0.44 +1.51 +1.05 +1.10 +0.20 +0.15 +1.05 V-B +0.05 +1.30 +0.60 +0.72 +0.15 +0.31 +0.56 +0.64 +1.00 +0.21 +0.03 -0.02 U-B RefRemarks ROB ROB NRS ROB ROB ROB Cn NRS Cn Cn Cn Cn mem?* =Eg B =ROB IV-112* -SG 13-43 -SG A* =Ao 260 =SG 10-60* mem* 2 obs. fid, -EgC -SG 15-5 -Ao 1* -SG 11-21 -SG 3-73* fid* -SG 9-61* -Ao 161 -Ba d* -SG 9-68* * -SG 12-12* fid? fid* fid* fid, -Bab* fid, -Baa* 198lApJS. ROB 662 NGC 6397(Continued) ROB 692 ROB 685 ROB 679 ROB 669 Primary IDAlt ROB 387=*CPD-53°8715 ROB 693 ROB 681 ROB 666 ROB 318=SG3-14=CPD-53°8723 ROB 713 ROB 698 ROB 694 ROB 44=Eg37 ROB 5=V639Ara=HV615 ROB 211=ROBIV-272=CPD-53°8728=CoD-53°7350 ROB 162=SG2-18 ROB 99=CPD-53°8709=»CoD-53°7343 ROB 43=EgZ Remarks; ROB 283=CPD-53°8722 ROB 251“EgV ROB 226=CPD-53°8732=CoD-53°7353 ROB 70=ROBIV-274 ROB 48=ROBIV-105=Eg57 © American Astronomical Society Ao C Ao F Ao A CS A13 CS 1 CS 5 CS A20 CS All CS 4 CS A9 CS A7 CS A2 CS A1 CS 7 CS 6 CS 2 CS A4 CS A3 CS A21 CS A17 CS A16 CS A10 SG 15-32 CS A18 + 24 + 17 + 22.67 + 60 + 34 + 22.6 + 14 + 7 + 22.9 + 19 + 27 + 21.2 + 22.48 + 43 + 47 + 69 + 21.1 - 83 + 96 + 81 + 61 +118 + 23 - 36 - 87 - 35 - 56 - 17 - 34 - 57 - 3 -102 Av 49 49 31 27 31 34 49 49 49 32 49 10 10 31 49 59 59 15 59 59 70 70 59 59 59 0.92 3.7 1.0 0.99 2.1 9 2.5 Ma Ma Ma Ma Ref DC& DCS DC& CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS SR 16.0 22.7 1.00 0.10 0.029 0.14 7.30 Provided bythe NASA Astrophysics Data System Wt 0.041 1.00 0.10 0.041 0.029 5.02 0.020 0.041 0.029 5.02 5.06 0.029 0.020 0.029 0.096 0.041 0.029 0.029 0.041 318 AO AO AO A1 Gp Gp AO A2 AO AO A3: A1 AO Gp Gp KO III F6 (V?) AO AO AO Gp Gp Sp ROB 666=SG16-1 ROB 661Thisstarismisidentified onthechartby ROB 644»HD159988=CPD-53°8710 =CoD-53°7344 ROB 627=HD160177=CPD-53°8730=CoD-53°7351 ROB 669»CPD-53°8716 ROB 603=CPD-53°8714 ROB 531=SG10-60 ROB 468“EgM ROB 436=SG9-10 ROB 447=CPD-53°8705=CoD-53°7340 ROB 428=Eg22 ROB 469“EgX=SG9-60=CPD-53°8708»CoD-53°7342 Ref CS HC CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS CS SR 10.28 +1.50+1.12ROB 11.17 +1.17+1.06Cn 12.64 +0.59+0.12Cn 13.6 10.7 +1.28+0.87ROB 13.4 +0.09+0.23ROB 12.01 +0.97+0.45Cn 13.07 +0.16+0.20NRS 10.50 +1.28+0.96Cn 11.28 +0.62+0.40ROB 9.07 +1.17+1.08Cn Cannon (1974).(AlcainoIisindicated) +0.02 +0.18ROB V-B U-B RefRemarks mem?* =ROB IV-70* =SG 16-11* =SG 15-12* fid fid* fid* fid 198lApJS ... 45. .259W M References: Hu NGC 6440 DW Demers&Wehlau(1971) References: V 2 V 17 V 7 V 1 E Edmondson(1935) Remarks: NGC 6402(M14) Ao Alcaino(1977b) J Joy(1949) DC& DaCosta,Freeman,Kalnajs,Rodgers,&Stapinski(1977) References: ROB 694“CPD-53°8735 CS Ciarla&Stock(1977) ROB 693“SG15-36 ROB 681“HD160133=CPD-53°8727“CoD-53°7349 Int Cn Cannon(1974) Int Ba Bailey(1902) Int F Feast(1966) Primary IDAlt3D Eg Eggen(Woolley,etal.1961;Harding,1971) NGC 6397(Continued) American Astronomical Society •Provided bythe NASAAstrophysics DataSystem Mayall (1946) Humason (1934) (a) MeanofmeasurementsbySlipher(unpublished)and Edmondson + 9 - 73 +150 -130 - 97 -148 -175 - 18 - 6 -129 - 75 -115 -183 -153 -124 -136 -101 -120 -115.3 - 90 -104 -149 -106 -125 -150 + 13 + 13 + 10 + 2 + 2 + 13 - 6 - 8 - 0 - 3 Áv 12 12 33 33 33 33 33 50 10 23 28 28 23 17 28 18 33 33 28 12 33 23 37 33 4.3 vdB M M vdB M M M Hu M vdB M M M M E Ref 0.19 0.13 0.13 0.19 0.13 0.31 Wt 319 0.094 0.68 0.68 0.094 0.094 0.094 0.040 0.27 0.11 0.094 0.094 0.094 0.86 0.094 0.19 F8 G2 G2e F5 G2 GO F8 Sp vdB vdB M Ma Mallia(1975) ROB Woolley,Alexander,Mather&Epps(1961) CS 6“CPD-53°8736=CoD-53°7355 NRS Newell,Rodgers&Searle(1969) ROB 698“Eg54=CPD-538726=CoD7348 HC Houk&Cowley(1975) Kin Klnman(1959) (b) CorrectiontoEdmondson*svelocity SR Searle&Rodgers(1966) SG Swope&Greenbaum(1952) Ref van denBergh(1969) van denBergh(1969) Mayall (1946) <14.81> <+1.22> <14.80> <+1.26> <15.645x40.77> <14.06> <+1.32> V-B U-B RefRemarks DW DW DW DW 0.8 0.9 0.94 0.3 0.5 0.3 0.6 fid (b) (a) 198lApJS ... 45. .259W NGC 6441 Primary IDAltAveRefWtSpVV-BU-BRemarks M Mayall(1946) References: Remarks: HS Hesser&Shawl(1977)SHSSmith,(1976) Int Remarks: NGC 6522 Int (a)Meanof3observations,includingprecedingentry, References: NGC 652a. Cb Clube(1965)vdBvandenBergh(1969) vdB vandenBergh(1969) Int (a)MeasurementbyHarding Int Reference: NGC 6541 SHS Smith,Hesser&Shawl(1976) Reference: Int Kin Kinman(1959) Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem (b) MeasurementbyG.Illingworth (b) MeasurementbyD.S.Evans + 16 + 10 + 22 + 12 + 54 - 80 - 64 + 57 - 78 - 59 + 32 + 29 + 26 - 25 - 43 +129 -156 -166 -152 -115 -171 -148 + 13 + 13 + 13 r 15vdB0.45 r 12vdB0.68 20 12 16 33 33 33 33 46 30 12 11 13 13 13 14 11 4 7 8 7 M M M M HS HS HS vdB Cb Cb Cb SHS SHS SHS Kin Kin Kin Kin Kin Kin 320 6.25 0.25 0.39 0.11 0.69 2.04 0.69 0.59 0.047 1.56 2.04 0.59 0.51 0.59 (a) (b) (b) (b) (a) 198lApJS ... 45. .259W M Mayall(1946) V 4 NGC 6626(M28) Reference: NGC 6624 vdB vandenBergh(1969) Reference: Reference: Kin KInman(1959) Reference: NGC 6553 Primary IDAltAveRefWtSpVV-BU-BRemarks Int Int Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Ma yall(1946) + 32 + 7 + 25 + 7 + 10 + 62 + 58 +210 +105 + 50 + 42 +184 +245 +114 + 3 - 25 - 8 - 15 - 26 - 4 -52 +13r13vdB0.59 -40 +13r13vdB0.59 - 34 - 9 0 23 43 23 33 32 33 33 33 33 23 37 33 33 33 33 77 33 33 73 61 57 33 33 M M M M M M M M M E Kin Kin Kin Kin Kin SI 0.19 0.19 321 0.090 0.094 0.094 0.094 0.094 0.094 0.19 0.094 0.094 0.094 0.017 0.094 0.019 0.027 0.054 0.094 0.094 0.094 0.031 0.094 G3 G4 0.42 0.16 =HV 620 198lApJS ... 45. .259W M Mayall(1946) NGC 6637(M69) References: NGC 6642 LM LloydEvansandMenzies(1971) References: Remarks: Remark: NGC 6626(Continued) vdB vandenBergh(1969) Reference: Reference: NGC 6638 HSg Hartwick&Sandage(1968) HSg 2-III-3Adoptedephemeris:Max=JD2435662+195E,after HSg 3-1-43V4 HSg 2-III-3?V5 Primary IDAltAveRefWtSpVV-BU-BRemarks CFM Catchpole,Feast&Menzies(1970) Int -103 +13 r11vdB0.83 Int -2733M Int Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Combination ofSlipher'svelocitywithremeasurement Joy (1949) Edmondson (1935) of sameplatebyEdmondson. misidentified onthechartbyHartwickandSandage Rosino (1962)andHogg(1973).Thisstaris that thephotometryreferstovariable. (Catchpole, Feast&Menzies1970);itisnotcertain +24 33M + 32.80 + 733M + 31e + 30e + 61e + 55e + 62e + 58e + 64.9 + 31 + 39 +158 + 97 + 90 + 89 - 5533M - 2033M + 13 ap ap ap ap ap ap 10 11 10 14 10 14 10 33 33 33 33 33 1.5 0.51 M M M M M vdB CFM CFM CFM CFM CFM CFM 0.77 0.77 0.78 0.44 0.44 0.78 1.97 2.05 0.094 0.094 0.76 0.094 0.094 0.094 0.094 0.094 0.094 0.094 322 Me Me M Mayall(1946) M vdB vandenBergh(1969) Ro Rosino(1962) SI CFM CFM Mayall (1946) Slipher (1918) 13.29V +1.99 13.22v +1.79 LM HSg 0.3 0.1 0.4: 0.3 0.2 0.6: =V1894 Sgr =Ro VI0* 198lApJS ... 45. .259W M Mayall(1946) NGC 6656(M22) Cv 358 Cv 274 Cv 243 Cv 223 Cv 179 Cv 165 Cv 139 Cv 382 Cv 359 Cv 283 Cv 278 Cv 232 Cv 213 Cv 158 Cv 101 Reference; NGC 6652 Cv 164 Cv 135 Primary IDAltAveRefWtSpVV-BU-BRemarks Int Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem AM III-110 AM III-78 AM III-47 AM III-108 Am 11-44 AM 11-94 LE 11-103 V 5 AM III-106-138.3 V 9 AM III-97 V 8 AM III-33 AM III-109 Kin 2 AM 11-23 Kin 1 + 6 + 7 + 26 -129.9 -159 -156.1 -139 -134 -120 -149 -135 -215 -149 -157 -105 -144 -133 -157 -158 -156 -100 -139 -124 -135 -146 -134 - 30 -151 -120 -122 -139 -160 -146 - 91 -148 -170 -105 -129 -135 -158 -160 -170 -146.9 -153.0 -154 -173 + 13 - 0 10 13 10 10 10 12 11 13 13 18 13 10 13 26 24 18 18 23 12 16 23 23 33 33 33 33 33 33 37 33 33 4.9 8 8 8 8 4.6 8 8 8.3 8 8 3.8 6 3.9 6 Ma LEI Ma M M M Kin LEI LEI Kin LEI LEI LEI MN M M M M M J HHa Kin HHa HHa vdB M LEI J LEI LEI J HHa J J J HHa J E 1.56 1.00 2.78 2.78 1.00 1.56 0.69 0.19 0.84 0.56 0.56 0.59 0.59 0.59 0.30 0.29 0.18 0.29 0.66 0.97 0.68 0.094 0.094 0.094 0.53 0.66 0.53 0.89 0.15 0.64 0.91 0.97 0.094 0.094 0.094 0.094 0.38 0.094 0.13 323 GO G6e CH G2 G5 G5e G2 G5e G2 G2e G5 MN J J J <11.21> <+l.92><+1.99>Eg <10.79> <+l.63><+1.38>Eg <10.90> <+1.73><+1.56>Eg 13.21 +1.28HHM 12.19 +1.49 11.85 +1.13HHM 12.34 +1.44 12.65 +0.49 11.01 +1.82+1.76Eg 12.53 +1.24HwH 12.98 +1.32LE 11.16 +1.79+1.575Eg 12.28 +1.25HwH 12.99 +1.16 12.19 +1.31HwH 12.10 +1.45LE LE LE HwH HHM 0.7 0.50 0.29 0.8 0.0 0.57 0.7 0.6 .=Ao 2-23 mem* =Ao 2-9* =Ao 3-16* 2 obs.(b) =Ao 1-17* =Ao 1-22* =Ao 3-59 =HV 633 =Ao 1-40* =AM III-3 =Ao 1-3 =AM III-14 fid?* fid fid fid* fid* (a) 198lApJS. NGC 6656(Continued) Primary IDAlt Cv 431AMIII-32 Cv 594 Cv 510 Cv 461V11 Cv 630 Cv 567 Cv 566 Cv 761 Cv 826 Cv 803 Cv 658 Cv 831 Cv 702 Cv 964 Cv 836 Cv 960 Remarks : Cv 910 Cv 158=HV630 Cv 135==HV634 Cv 101“Ao3-56 Cv 179=HwH4807 Cv 164=Bad=ZNG5 Cv 223-HwH5707 Int (a)MeasurementbyHumasen. Cv 274=HwH3807 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem (b) RevisionoffirstentrybyEdmondson AM IV-29 LE V-4 AM IV-26 AM 1-98 Kin 3 AM IV-24-183.2 AM IV-52 AM IV-72 LE 1-106-171 AM 1-36 AM IV-67 AM 1-92 AM III-ll V 14 LE IV-108 AM 1-62 AM IV-54 LE IV-107 HwH 8909 HwH 1809 -146 -135 -165 -158 -144 -149 -144.2 -183 -157 -139 -175 -147 + 43 -164 -154.0 -195 + 58 + 63.6 + 12 -141 -180 -179 -133 -188 + 57 -151 -167 -148 -148 -179 -173 - 35 -172 - 17 -120 -176 -208 + 1 + 9 - 16 + 7 + 6 Av ap 23 ap 18 13 13 11 23 10 12 10 12 16 10 22 10 11 11 11 11 5.1 8 8 8 5.0 9 8 5 9 8 9.6 6 8 8 1.3 7 5 6 9 Ref LEI HHa LEI HHa HHa HHa Kin J J J LEI HHa HHa LEI HHa HHa HHa LEI HHa LEI LEI HHa HHa HHa HHa HHa HHa HHa HHa HHa 0.61 0.63 0.18 4.00 1.56 1.56 1.00 2.78 4.00 1.00 1.56 0.69 1.00 2.78 0.83 0.28 0.18 Wt 0.87 0.66 0.59 0.59 0.88 0.53 0.17 0.28 0.41 0.59 0.48 0.73 324 A8 F2 CH? FO CH M5e M3.5e Sp Cv 278=Ao3-81 Cv 702=HwH7906 Cv 594=Ao1-47=HwH7904 Cv 431=HwH6811 Cv 359=HwH6807 Cv 358=Ao3-82 Cv 831=HwH1907 Cv 658=HwH7703 HH Ref HHa H.61 +1.48+1.26Eg 11.37 +1.63 13.84 +1.08 12.40 +1.27+0.865Eg 14.44 +0.28 14.01 +0.99 14.09 +0.91 12.46 +0.97 12.63 +1.28 12.33 +1.24 11.75 +1.33 11.42 +1.29LE 14.35 +0.96 12.16 +0.79 12.12 +0.77+0.07Eg 12.39 +1.19HwH 14.25 +0.98 14.39 +1.00 14.39 +0.99 12.89 +1.44 V-B U-B RefRemarks LE LE HwH HwH HwH HwH HwH =HwH1605 HwH =Ao1-51 HwH LE LE HwH HwH HwH HwH 0.79 0.38 0.20 0.25 0.11 mem* mem* =HV 636 mem* =HwH 7803 =LE V-5 =HwH 2811 mem* =HwH 1708 =Ao 1-78* mem =HwH 5601 =HwH 7907 fid* fid, =ZNG11 fid* fid* fid* 198lApJS ... 45. .259W Kin Kinman(1959) References: M Mayall(1946) NGC 6715(M54) References: M Mayall(1946) F Feast(1967) Ao Alcaino(1977a) NGC 6712 Reference: NGC 6681(M70) AM Arp&Melbourne(1959) References: HwH Hartwick&Hesser(HesserHarris1979) NGC 6656(Continued) Int SSm Sandage&Smith(1966) HHa Besser&Harris(1979) SSN Sandage,Smith&Norton(1966) SSm C26ZNG1 Int HHM Hesser,Hartwick&McClure(1977) Eg Eggen(1977) E Edmondson(1935) Cv Chevalier(1918) Ba Bailey(1902) Cv 836=HwH8805 Primary IDAltvAveRefWtSpVV-BU-BRemarks Cv 960=Ao3-128 Cv 910=Ao2-46=ZNG2 Int r © American Astronomical Society • V 7 +136 +124 +139 + 86 +100 +131 +131 + 95 +219 +203 +154 +218 -125e -123.0 -139 - 67 -155 -123 e -152 -175 -127 + 13 ap ap 19 33 33 33 33 12 33 33 33 33 33 33 33 33 8 5 7 1.1 9 SSRI M M M M M Kin Kin Kin M M M M vdB 1.19 1.19 Provided bythe NASA Astrophysics Data System .0.094 4.00 1.56 2.04 4.36 Me 0.094 0.094 0.28 0.094 0.68 0.094 0.094 0.094 0.094 0.094 0.094 0.094 0.094 325 A (I?) V 14=V1311Sgr vdB vandenBergh(1969) Cv 964=Ao3-129=ZNG3 MN McClure&Norris(1977) Ma Mallia(1976) M Mayall(1946) LEI LloydEvans(1978) LE LloydEvans(1975) Kin Kinman(1959) ZNG Zinn,Newell&Gibson(1972) vdB vandenBergh(1969) SSRI Strom,Rood&Iben(1970) J Joy(1949) ZNG Zinn,Newell&Gibson(1972) F <12,72><+1.94> SSRI 13.14+0.42 Mayall (1946) SSm SSN 0.96 0.93 mem, 2obs. =CH Set 198lApJS ... 45. .259W Remark: NGC 6723 References: Primary IDAlt3DAv£RefWtSpVV-BU-BRemarks Ao Ao 16 NGC 6779(M56) References: Int CS Int KU 337 KU 284 Int American Astronomical Society •Provided bythe NASAAstrophysics DataSystem Mayall (1946) Alternative velocity-98±12km/spossible. Alcaino (1972) Cannon &Stobie(1973) Kin 1 V 3 V 6 Kin 3 Kin 4 Kin 2 ‘"'-133 + 56 + 1 + 16 + 8 - 37 - 48 - 51 -125 - 26 - 44 - 45 - 32 - 30 -201 -188 - 56 - 37.3 - 29 - 6 -130 - 39 - 37.55 - 31 -129 -210 - 40 -154 -147 -160 -121 -156 -155 -118 -137 -123 -127 -135 -128 -131.0 -168 + 7 + 7 + 7 + 7 + 7 12 17 33 13 13 13 13 12 10 33 33 33 18 10 13 23 23 23 18 18 18 23 13 33 33 33 23 33 33 4.9 8 5 9 6 3.0 6 9 6 0.50 M M M M LE Kin Kin Kin Kin Kin Kin Kin Kin Kin Kin Kin SHS 0.30 0,30 0.19 0.30 0.47 0.17 0.47 4.00 0.26 0.17 0.47 0.47 0.17 0.47 2.78 1.23 0.17 0.47 2.78 2.78 0.69 326 1.23 1.56 2.78 0.094 1.79 2.11 0.69 0.094 0.094 0.094 0.76 3.16 3.40 0.094 0.094 0.094 0.80 M3 GOe G2 F6 GO F8 G2 G2 G2 GOe F8 GO G4e GO G2 G3 LE Kin SHS LE Lloyd Evans(1977a) Smith, Besser&Shawl(1976) Kinman (1959) <12.67> <+1.28> <12.75> <+1.82> 11.53 +1.56+1.78CS Bb Bb 0.39 0.08 0.86 0.58 0.48 0.26 0.07 0.02 0.80 0.60 0.28 0.24 0.16 0.91 0.53 mem? =vM 125* =vM 137* 198lApJS ... 45. .259W S 153AH77 NGC 6838(M71) References: CSr HSt 2 HSt 3 HSt 1 Ao S 150AH78 Int Pal 11 Kin Lee 4406 References: Lee 4505 Lee 2502 Lee 1518 Lee 2437 NGC 6809(M55) References: Remarks: Int Kii Kii 284=RoA-l KÜ 363 NGC 6779(Continued) Bb J E Int MeasurementbyHumason. Primary IDAlt American Astronomical Society •Provided bythe NASAAstrophysics DataSystem Canterna &Schommer(1978) Alcaino (1975c) Kinman (1959) Küstner (1920) Barbon (1965) Edmondson (1935) Joy (1949) Kin 1 Kin 4 Kin 2 Kin 5 Kin 3 V 1 - 16 - 60 - 5 - 55 - 19.0 - 55 -144 +160 - 62 - 86 +163 +126 - 58 - 75 - 51 +179 +171 +175 -186.0 -178 -166 -201 -157 + 1 + 1 + 1 + 1 + 1 + 13 - 11P18 14 Av 19 12 40 15 33 33 33 33 40 HSt 28 HSt 28 HSt 13 23 18 23 1.3 8 5 6 7 9 4.4 GN M M M M GN HSt JK Kin Kin Kin Kin Kin vdB Ref 0.69 0.062 0.30 0.18 0.30 0.19 Wt 59.2 0.27 0.094 0.094 0.094 0.12 0.062 0.12 1.94 1.26 2.47 1.04 1.55 0.59 327 A6 A8 F8 G5 Sp HSt vdB Lee M Mayall(1946) vM vanMaanen(1927) Ro Rosino(1951) KÜ 337=Ro961.Adoptedephemeris:Min=JD2428015.8 Ref Hartwick &Sargent(1978) Lee (1977c) van denBergh(1969) <15.50> 12.51 +1.96 12.73 +1.59 11.39 +1.37+0.98Lee=Ao575 11.63 +1.35+1.09Lee=Ao454 11.79 +1.30Lee=Ao516 11.84 +1.27Lee=Ao626 11.77 +1.29+0.94Lee=Ao538 + 101.67E(Joy1949). V-B U-BRefRemarks Cw Bb Cw 0.87 0.86 0.91 0.74 =CSr 12A =CSr 33 fid?* mem, =Ro864 =At 848* 198lApJS ... 45. .259W NGC 6838(Continued) Primary IDAlt S 184 S 176AHA S 189 S 201 S 185 Remarks: S 262 S 217 S 227 S 226 S 222 S 211 S 249 S 150=At849.PhotometrybyGuffey(1973)andCudworth(1976) At Artiukhina(1956) AH Arp&Hatwick(1971) S 184=At891.(seealsoremark,150). S 176=C5=HDE350790.(seealsoremark,150). S 153(seeremark,150). References: HDE Cannon&Mayall<1949)[HenryDraperExtension!] S 189=At905 S 185=At898.(seealsoremark,150). Hb Herbig(1960) C Cuffey(1973) S 201=At909.Possiblyvariable.Thereisasubstantialresidual HSt Hartwick&Sargent(1978) GN Gratton&Nesci(1978) NGC 6864(M75) Cw Cudworth(1976a) Int American Astronomical Society •Provided bythe NASAAstrophysics DataSystem AH 113 AH 45 AH 64 AH 36 AH 30 AH 46 V 1 AH 49 AH A1 AH W V 3 AH V Hartwick (1971)by0.11mag,average,atV. is systematicallybrighterthanthatofArpand and thatofCudworth(1976).(seealsoremark,S150). difference betweenphotometrybyArpandHartwick(1971) - 29 - 26.8 - 17 - 24 - 16.5 - 21 - 24 - 9 - 16 - 10 - 11 - 20.6 - 19 - 15 - 18.2 - 18 - 22 - 20 - 55 - 72 -222 -229 -232 -224 22 29 26.4 - 16: Av 40 40 18 11 10 18 14 11 14 28 20 15 14 11 33 33 33 19 3.6 3.4 7.5 5 3 1.9 5 1.6 Ref PS GN GN GN GN HSt HSt GN GN GN GN GN GN GN PS Li PS PS M M M M 0.83 0.062 0.31 0.062 0.51 0.31 0.44 0.83 0.47 0.12 Wt 2 2 8.39 0.49 0.77 3.00 0.92 1.55 5.05 9.19 5.78 0.094 0.094 0.094 328 MO: F5 FO gM6 B8 Sp Kg Krug(1936) S 217=At937 S 211=At923=Sp2 PS Pike&Stickland(1977) M Mayall(1946) Li Liller(1978) JK Jenner&Kwitter(1977) S 262=HDE350789 S 227=Kg40=Sp1=ZSge S 226=At948=C13.(seealsoremark,150). S 222=At949=C12.(seealsoremark,150). S 249=C1=HDE350788=BD+18°4292.(seealso Sp Stephenson(1961) S Sanders(1971) Ref HDE 10.6740.49-0.08C Hb Sp HDE 11.31+0.3340.23AH HDE 10.04+0.08-0.57C 12.35 +1.91Cw 12.91 +1.66 12.06 +2.06Cw 12.53 +1.45AH 12.09 +1.74 12.34 +1.82 11.99 +1.33+1.45C 12.76 +0.26-0.16C 12.97V +1.65 15.11V +0.46 remark, S150). B-V U-B RefRemarks AH AH Cw AH AH 0.9:fid,=AH255 =Kg 14* =Kg 18* fid?, =Kg12* =Kg 22* fid, =At896* =Kg SI* =AH 27* =Kg 39* =Kg 38* =Kg 36* =At 1013* fid, =At990* 198lApJS ... 45. .259W M Mayall(1946) HSt Hartwick&Sargent(1978) References: Hu Humason(1934) NGC 7006 Hu References: HS NGC 6981(M72) M Mayall(1946) References: Remarks: SWy II-4 Kin SWy 11-46 Int E Edmondson(1935) References : NGC 6864(Continued) Int Primary IDAltv.AeRefWtSpVV-BU-BRemarks Int v © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Besser &Shawl(1977) Humason (1924) Kinman (1959) (a) RevisionbySlipher,basedon entry. -387 -368 -309 -230 -180 -416 -402 -407 -322 -394 -350 -281 -286 -269 -317 -182 -355 -416 -395 -266 -365 -350 -410 -189 -203 -158 -186 + 13 + 13 - 1 - 1 - 1 - 1 40 40 13 13 12 33 33 33 33 35 33 33 33 50 33 33 23 same plateasfirst 33 33 33 35 37 33 8 6 7 6 M M M M M vdB vdB M M M M HSt HSt Hu HS M M M Hu E Kin M Kin Kin Kin Sb SI 329 0.094 0.062 0.062 0.59 0.59 0.094 0.094 0.082 0.094 0.094 0.094 0.094 0.69 0.040 0.094 0.094 2.78 1.56 0.094 0.19 2.04 0.094 vdB SWy Sb Strömberg(1925) SI Slipher(1918) (b) CombinationofSlipher'srevisedvelocitywith measurement ofsameplatebyEdmondson. Mayall (1946) van denBergh(1969) Ma yall(1946) Sandage &Wildey(1966) 16.38 +1.33 16.62 +1.21 SWy SWy (b) (a) 198lApJS ... 45. .259W KU 64 NGC 7078(M15) KU 146SgS7 KÜ 29 KU 28 KU 553 KU 224 KU 169 KU 144 KU 70 KU 66 KU 731 KU 662 KU 648 KU 559 Kü 498 KU 476 KU 431 KU 387 Kü 156V1 KU 147AIII-34 KU 73 Primary IDAlt KÜ 757 Int Kil 609 KU 575? Kü 761 American Astronomical Society •Provided bythe NASAAstrophysics DataSystem A 11-30 A 11-75 A III-67 A 11-64 A IV-38 A 1-63 ZNG 3 A IV-63 Ps 1 ZNG 1 Sg PI3 Sg S37 Sg X6 Sg X5 A IV-40 Kin 1 Sg S36 Sg P6 Sg Sll Sg S3 Sg P14 Sg SI + 26 -107 -122 - 35 -125 -180 - 93 -100 - 96 -105 -120.3 -120.0 -103 - 87 -135 - 77 -110 - 95 - 22 -109 -162 -111 -124 -124 - 97 - 72 -114 - 97 -159 - 86 -120 -129 -107 -113 -100 - 78 - 86 -138.9 -116 - 93 - 86 -118 - 92 - 95 -138 -117 -119 - 93 -121 -115 -156 -120.8 -126 + 20 + 2 - 8 - 12 - 12 - 12 - 12 - 12 - 12 - 12 - 12 - 12 12 12 12 12 12 12 Av •33 40 18 40 18 10 18 19 19 18 10 10 20 16 13 20 10 20 20 20 20 20 20 20 20 20 33 33 35 37 10 10 18 18 35 20 20 33 33 50 20 20 12 4 4 1.5 1.2 1.6 8 9 3.0 9 9 M M M M M Mo NZ M Ref NZ NZ Kin NZ NZ NZ NZ W NZ NZ 0.24 NZ NZ NZ Kin Kin NZ NZ HHa 1.00 Co HSt 44.4 NZ Kin Ps OPK J J HSt HSt Z Gr E SSRI Co OPK J Z Gr J Gr Ps Sb SI 0.29 0.31 1.00 6.25 0.32 0.32 0.082 0.062 6.25 0.062 Wt 1.23 1.56 1.54 1.00 0.48 0.31 0.094 0.094 0.28 0.094 0.38 0.66 1.51 0.21 0.094 0.094 0.040 0.28 0.21 0.21 0.21 0.21 0.21 0.21 0.21 0.43 0.61 0.21 0.21 0.21 0.61 0.21 0.61 330 B9-A0 III-VSSRI A8 wkGbd wkGbd Neb F0 F8 V Sp Ref NZ NZ OPK <14.89> <+0.28>Al 13.78 +0.57Br 13.72 +1.02+0.58Sg 14.11 +1.01+0.45Sg 14.89 +0.85+0.37Sg 14.32 +0.97+0.43Sg 15.33 +0.82+0.26Sg 14.93 +0.90+0.21Sg 14.68 +0.88+0.28Sg 13.24 +1.14A 13.48 +1.12+0.76Sg 12.56 +0.61A 13.54 +1.08+0.66Sg 13.01 +1.26+0.98Sg 14.39 +0.91+0.40Sg 15.01 +0.14 12.72 +1.25 14.12 +0.94 14.06: -0.33:Br 14.80 -0.20Z 15.93 +0.17+0.20Sg 13.02 +1.20+0.94Sg 13.45 +1.09+0.70Sg 16.06 +0.08+0.09Sg V-B U-B RefRemarks A A Co 0.99 0.37 2 obs.* =B 53 3 obs* 2 obs. 2 obs. fid mem?, =HV660 =B 4* =B 7* =B 3 2 obs.,(a) =*Ga 38* =B 25 =B 22 =B 6 =Ga 39* 2 obs. fid fid, =B5 fid (d) (e) (c) (b) 198lApJS ... 45. .259W NGC 7078(Continued) Kli 859 KU 914 KU 912 KÜ 882 KÜ 825SgS4 Primary IDAlt Kli 918 Remarks: KU 1082 KÜ 1040 KÜ 996 KU 1106 A Arp(1955b) References: NGC 7089(M2) A1 Arp(1955a) Ku 575Thisstarisidentifiedintheobservingnotebookonlyas KU 224°Ga47 KU 146*=Bac KU 144MeasurementbyGunnandGriffin. HSt Hartwick&Sargent(1978) Gr Greenstein(1968) Co Cohen(1979) KU KUstner(1921) Kin Kinman(1959) HHa Hesser&Harris(1979) Ga Gamalej(1948) E Edmondson(1935) Ba Bailey(1902) Int (a)CombinationofSlipher'svelocitywithmeasurementby HN Hesser&Nemec(1979) Br Brown(1951) B Barnard(1931) J Joy(1949) Int American Astronomical Society •Provided bythe NASAAstrophysics DataSystem (b) MeasurementbySanford. (e) MeasurementbyAdams. (c) MeasurementbyWright. (d) RemeasurementofWright’splatebyMayall. A IV-44 A IV-48 A 1-70 ZNG 2 Sg S23 Sg S16 Sg S6 Sg X2 Within thefieldofview(r=2!5)Radcliffe Edmondson ofthisplateandoneother. description ismostnearlyfulfilledbyKU575,but 76-in. reflectorattheCassegrainfocus,this the brightstaratnorthedgeofcluster. this identificationisnotcertain. -100 - 89 - 92 -114 -104 -104.00 - 71 -104.1 -119 -131 -122 -104 -125 -111 -131 - 64 -101 - 70 + 8 + 39 + 15 - 15 - 10 - 6 - 12 12 12 12 12 Av 40 20 20 40 40 20 11 20 13 10 10 28 10 33 10 33 37 33 10 19 8 8 0.00 5.3 Ref NZ NZ NZ NZ HSt HN NZ HSt HN HN M M HSt Z St St St M M E SI 0.59 0.062 0.062 0.24 0.062 1.00 1.00 1.00 Wt 0.54 0.21 0.39 0.21 0.39 0.58 0.12 1.09 1.57 0.094 0.94 0.094 0.28 0.094 331 wkGbd AO A3 Sp Mo Moore(1932) M Mayall(1946) KU 825“A1-12 KU 757=B56=Ga7.PhotometrybyHintzen. KU 1082Suspectedvariable(Chu1976).Adopted KU 914(seeremark,882). KU 761“ZNG7.Thisstariserroneouslyidentified KU 648=PK65-271.Planetarynebula. Ps Pease(1928) NZ Norris&Zinn(1977) KU 882Sargentlistsonlyacombinedmeanvelocityfor W Wallerstein(1958a) PK Perek&Kohoutek(1967) OPK O’Dell,Peimbert&Kinman(1964) ZNG Zinn,Newell&Gibson(1972) Z Zinn(1974) Sg Sandage(1970) Sb Strömberg(1925) SSRI Strom,Rood&Iben(1970) SI Slipher(1918) St Sargent(1967) Ref NZ HN 12.69 +1.37+1.29Sg 14.30 +0.84A 15.79 +0.25+0.18Sg 14.24 -0.07Z 14.01 +1.04+0.68Sg 15.96 +0.14+0.26Sg 16.84 -0.09-0.60Sg 13.40 +1.19+0.83Sg 15.05 +0.19 14.62 +0.97+0.40Sg + 0.087004E. as IV-50byStrom,etal.(Zinn1973b). ephemeris: Max=JD2436069.997 1-70 (KU882)andS16914). B-V U-B RefRemarks Br 0.1:-l.5: 0.7:-1.4: =Sg S18* =B 57* * =B 68 =B 71 fid, =B59 5 obs.* 198lApJS ... 45. .259W NGC 7089(Continued) A 1-59 Primary IDAlt A IV-96 A Arp(1955b) A IV-96 A 1-59 Remarks: Kin Kinman(1959) De Demers(1969,1971) Ha Harris(1975) References: Ga Gamalej(1948) NGC 7099(M30) J Joy(1949) E Edmondson(1935) Int Int © American Astronomical Society •Provided by theNASA Astrophysics DataSystem =ZNG 1 Combination ofSlipher’svelocitywithmeasurementby =vM 152 V 5 V 1 V 6 V 11 Ha 11-94 ZNG 2 Edmondson ofthisandfourotherplates. + 24 + 7 + 9 + 7 + 10 + 4 + 36 + 4 + 15 - 8 - 42 - 15 - 21 - 33 + 16 - 9 - 10 - 18 - 24 - 20 - 11 - 27 - 3 - 28 - 6 - 15 - 2 - 4 - 14 - 14 - 17 - 15 - 24 - 15 - 27 - 18 - 8 -155 -125 -163 -178 -147 -217 -128 7.4 0 + 5 + 4 + 1 + 10 - 15 - 9 + 13 + 11 + 10 + 10 + 11 + 4 + 4 + 8 + 12 + 11 + 11 + 8 + 8 + 7 - 5 + 2 - 5 - 5 - 12 - 1 - 7 - 6 - 12 - 9 - 1 - 15 Av 11 13 13 19 18 18 18 13 13 13 13 18 18 18 23 15 23 28 12 33 13 18 18 13 18 18 18 13 13 13 18 13 13 23 28 19 23 33 37 33 33 33 5 2.0 M Ref vdB Kin Kin Kin SSRI M M SSRI M M M E SI 0.30 0.31 0.30 0.19 0.19 0.13 0.63 0.32 0.63 0.63 0.32 0.63 0.32 0.32 0.32 0.32 0.32 0.63 0.32 0.63 0.63 0.63 0.63 0.19 0.63 0.13 0.63 0.32 Wt 0.54 0.35 0.51 4.00 1.51 0.94 0.59 0.59 0.094 0.66 0.28 0.094 0.19 0.094 0.094 0.094 0.28 332 AO-2 III AO-2 III F6 F8 F6 G2e F8 F8 GO GO G3e G2 F6 F8 F6 GO GOe GOe GO F6 F8 F8 F5 F5 F5 GO GO F6 G2 G3 Sp V 11 V 5 V 6 M Mayall(1946) vM vanMaanen(1927) vdB vandenBergh(1969) ZNG Zinn,Newell&Gibson(1972) SSRI Strom,Rood&Iben(1970) SI Slipher(1918) Ref SSRI 15.19+0.06 SSRI 14.74+0.16 =Ga 15=HV716 =Ga 25’—HV715 »^HV 721 <13.46> <+0.525><+0.57>De <13.34> <+0.52><+0.51>De <13.18> <+0.54> <12.20> <+0.47> V-B U-B RefRemarks A De De Ha 0.86 0.32 0.91 0.15 0.21 0.19 0.04: 0.04 0.76 0.30 0.46 0.35 0.31: 0.27: 0.19: 0.85 0.84 0.76 0.69 0.69 0.66 0.64 0.63 0.58 0.43 0.42: 0.97 0.66 =vM 164* 4 obs.* =HV 711 2 obs.* =vM 144* =vM 113* 198lApJS. ^ PrimaryIDAltAveRefWtSpVV-BU-B C Guffey(1961b) References: NGC 7492 Bs Barnes(1968) HSt Hartwick&Sargent(1978) C RlSl-6 M NGC 7099(Continued) Reference: References: Remark: Reference: Kin HSt Hartwick&Sargent(1978) HSt 1+8 HSt 5+44 HSt 3-26 Pal 12(Capricorn) E HSt 2-65 Pal 13(Pegasus) Int CombinationofSlipher’svelocitywithmeasurement CSr Canterna&Schommer(1978) © American Astronomical Society •Provided by theNASA Astrophysics DataSystem Mayall (1946) Kinman (1959) Edmondson (1935) same platebyEdmondson. -197 -180 -188.5 -198 -204 -171 -169 -196 + 13 - 0 - 0 - 0 - 0 40 HSt0.062 40 HSt0.062 40 HSt0.062 40 HSt0.062 40 40 17 13 28 8.5 4 3 vdB HSt HSt Kin Kin Kin Kin 11.1 333 1.35 0.062 0.59 0.062 0.13 0.35 vdB HSt Hartwick&Sargent(1978) SI van denBergh(1969) Slipher (1922) 15.64 +1.06Bs Remarks CSr 14 198lApJS ... 45. .259W References: Hg 97 For 4 For 3 Hg Ursa Minor DDHW Danziger,Dopita,Hawarden&Webster(1978) Primary IDAlt Remarks: vA 230 vA 177 Remarks : For 5 HMS Humason,Mayall&Sandage(1956) References: Sculptor References: PN Draco vA 177 References: HSt HSt Hartwick&Sargent(1978) BSw 75-267 BSw 45-24 BSw Baade&Swope(1961) Sn Stetson(1979) © American Astronomical Society •Provided bythe NASAAstrophysics Data System Hodge (1965) Hartwick &Sargent(1978) It isextremelyunlikelythatbothvA177and230are (a) For3,4,and5areglobularclustersatellitesof (b) Meanofthreeplates,includingthatMayall. NGC 1049+70 Fornax. Velocitiesrefertospectraofintegrated members ofUrsaMinor.Thestrongermetalliclines light. membership forthelatterstar,butnotconclusivelyso. color-magnitude diagram,supportthepresumptionof galaxies generally,andthepositionofvA230on the extremelylowmetallicityofdwarfspheroidal in vA177(Cowley,Hartwick&Sargent1978),given (asymptotic?) giantbranchinvanAgt’sinstrumental +196 + 59 + 35 + 43.2 + 85 + 63 + 40 + 30 + 32 - 25 -244 -105 -236 -305 + 13 + 13 + 13 + 13 + 13 CATALOG OFRADIALVELOCITIESINDWARFSPHEROIDALSATELLITESTHEGALAXY Av 80 HSt0.016 14 44 46 14 14 13 19 40 89 14 23 28 23 28 1.3 e RefWt M vdB vdB vdB vdB vdB HMS HMS HSt HSt HSt HSt 0.013 0.59 0.50 0.28 0.051 0.50 APPENDIX 2.05 0.50 0.42 0.061 Neb 0.19 0.19 0.12 334 Sp RefVV-BU-BRemarks vdB M HSt Hartwick&Sargent(1978) vA 230(seeremark,230). For 4(seeremark.3(a)). vA For 5(seeremark.3(a)). PN Planetarynebula. DDHW Mayall (1946) van Agt(1967) van denBergh(1969) 17.27 +1.71 17.13 +1.44 17.07 +1.30 Hg Sn 3obs. Sn 2obs. mem, 3obs.* fid?, 2obs.* (a) (b)