NCAR/TN-314+STR NCAR TECHNICAL NOTE
I- - - October 1989
HAO-Lowell-AFGL Solar Stellar Spectrophotometer Star Catalog
R. Gilliland K. Fisher D. Mihalas R. Fisher W. Lockwood R. Radick L. Ramsey
HIGH ALTITUDE OBSERVATORY
NATIONAL CENTER FOR ATMOSPHERIC RESEARCH BOULDER, COLORADO
HAO - LOWELL - AFGL SOLAR STELLAR SPECTROPHOTOMETER STAR CATALOG
TABLE OF CONTENTS
PAGE PREFACE v
1. INTRODUCTION 1.1. BACKGROUND 1.2. THE HAO-LOWELL-AFGL COLLABORATIVE PROGRAM 1.3. PROJECT SUMMARY 1.4. SELECTION OF CATALOG STARS
2. THE HAO-LOWELL-AFGL CATALOG 4 2.1. HAO# 2.2. RA 2.3. DEC 2.4. PMa 2.5. PM8 2.6. PARALLAX 2.7. V 2.8. B-V 2.9. U-B 2.10. R-I 2.11. I 2.12. SPECTRAL TYPE 2.13. RADIAL VELOCITY 2.14. HK FLUX 2.15. WOOLLEY # 2.16. BRIGHT STAR # 2.17. HENRY DRAPER # 2.18. SMITHSONIAN ASTROPHYSICAL OBSERVATORY # 2.19. BONNER DURCHMUSTERUNG # 2.20. FINDING CHART 2.21. BINARY 2.22. ABBREVIATIONS USED
3. ACKNOWLEDGEMENTS 8
4. REFERENCES 9
5. CATALOG 11
6. NOTES TO THE CATALOG 33
PREFACE
This catalog of stellar sources comprises the set of stars selected for the HAO-Lowell-AFGL Solar Stellar Spectrophotometry project The joint observing program, is being carried out by the High Altitude Observatory, a division of the National Center for Atmospheric Research, and the Lowell Observatory of Flagstaff, Arizona. There are six scientific collaborators, one from each institution, High Altitude Observatory (HAO), Lowell Observatory, Pennsylvania State University, the University of Illinois, the Space Telescope Science Institute, and the Air Force Geophysics Laboratory (AFGL). This list of stellar objects was used for the first time during the initial observing season, September to December 1988.
R. R. Fisher High Altitude Observatory Boulder, Colorado 1
SOLAR STELLAR SPECTROPHOTOMETER STAR CATALOG
1. INTRODUCTION
1.1. Background: The fascination of solar astronomers for phenomena resulting from solar magnetism started with Galileo's discovery of sunspots in 1610, and heightened with Schwabe's recognition in 1843 that the number of spots varied cyclically with an 11-year period. The foundations of the subject were laid by G. E. Hale early in the 20th century when he proved that sunspots are regions of intense magnetic fields, and enunciated his famous laws of spot polarities. Babcock's demonstration in the 1950's that the full solar cycle is, in fact, a 22-year cycle in which the global magnetic field undergoes regular reversals provided impetus for the development of a basic picture of magnetic field generation through a dynamo mechanism by Parker, Babcock, and Leighton. Extensive studies of the solar cycle, activity centers, and solar flares have taken place over the last two decades; nevertheless the broad picture of magnetic field generation is still incomplete. Many details still remain obscure, and the questions of how magnetic fields emerge and dissipate undoubtedly require observations at the highest possible spatial resolution. There is, on the other hand, little doubt that on the large scale some kind of dynamo is in operation, and the development of reliable models for the dynamo is one of the outstanding challenges in modem solar physics.
1.2. The HAO-Lowell Collaborative Program: A team of scientists from the High Altitude Observatory, Lowell Observatory, Air Force Geophysics Laboratory, Pennsylvania State University, the University of Illinois, and the Space Telescope Science Institute have constructed an optical-fiber fed spectrograph with state-of-the-art detector systems to measure stellar fluxes in (1) the Call H and K lines, (2) the hydrogen Ha line, and the (3) Call infrared triplet lines. The highly automated system has been designed with emphasis on stability and ease of use for the observing crew. The Call H and K lines are known from existing work to provide a high-contrast chromospheric signal. The investigators plan to cross check the data against Mt. Wilson observations. The other two absorption features provide new information, and are located in spectral regions where most of the flux emerges in cool stars. Thus, the investigators expect to be able to observe both fainter and cooler stars than has been done previously in a synoptic stellar activity program. It is hoped that it may be possible to push the observations to stars that are wholly convective (unlike the Sun which has a convective envelope but has a radiative core), and thus explore whether there is a qualitative difference in the nature of the dynamo process for stars with an internal structure fundamentally different from that of the Sun. Finally, it is known that Ha provides information about stellar flare activity. The spectrograph is fed by the 1.1 meter telescope of Lowell Observatory in Flagstaff, Arizona. A description of the goals, observational approach, mode of operation, and the scientific products of this project are summarized below. Basically, we plan to operate in both a "survey mode" to determine long-term cyclic behavior for a wide variety of stars (observations made for a few nights every month of the year), and an intensive "rotation mode" to measure rotation rates for a subset of this larger sample At the same time, direct solar observations with the same set of equipment will be taken so that the behavior of a known rotating, magnetic star can be injected into the data stream. 2
1.3. The Solar Stellar Spectrophotometer Project Summary:
Scientific Goal: To understand the origin of magnetic activity cycles in lower main sequence, solar- type stars as a function of stellar age and other physical attributes.
Observational Approach: To observe spectral features known from solar and stellar studies to be indicators of magnetic centers of activity (e.g., plage). Specifically, we measure line to continuum ratios for Call H and K, Ha, and the Call IR Triplet. The Call lines are known to be in emission in plage; Ha is known to be sensitive to flare activity. The behavior of the Call IR triplet is known to correlate closely with the Call H and K lines (Herbig 1985); we hope that the IR triplet will remain useful for later types of stars than can be accessed with the H and K lines.
Data Needed to Achieve Goal: 1. Long-term synoptic coverage of line-index variations to determine existence and morphology of cycle for each star under study. (Time scale: 2-20 years).
2. Medium-range intensive coverage to allow inference of rotation periods from rotational modulation of signal. (Time scale: 2-50 days).
Modes of Operation: 1. Survey mode: A few good observations per month, through entire observing season, for a large number of stars to map out cyclic behavior for a wide range of spectral classes and population groups.
2. Rotation mode: Near-nightly observations of a selected set of stars over a period of 120 days per year, sufficient to establish rotational modulation unambiguously.
Information to be Inferred from Data: 1. Cycle morphology as a function of age, rotation, mass, composition.
a. Regular cycles vs. stochastic. Classes of cycles (rise-time to decline-time ratio). b. Existence of "Vaughan-Preston gap".
c. Behavior of cycle in late spectral types. Specific question: Does nature (or existence) of cycle change when star becomes fully convective?
d. Behavior (and/or existence) of magnetic activity in a variety of stellar population groups: young disk, old disk, halo.
e. Existence (?) of magnetic activity and/or cycles in subgiants.
2. Rotation periods. Differential rotation rates if possible.
3. Existence (?) of preferred longitudes of activity.
4. Correlation of cycle morphology and flare activity.
5. Growth and decay of active regions.
6. Radial velocity variations: (a) rotational modulation; (b) orbital modulation. 3
1.4. Selection of the Catalog Stars: The primary goal of this catalog is to provide the HAO-Lowell-AFGL Solar Stellar Spectrophotometry project with an unbiased list containing about 400 stars suitable for the observational study of magnetic activity in late-type stars. Simultaneously, this catalog is meant to provide other groups of investigators a list of candidate stars to examine in their own programs, carried out in parallel with ours. The ultimate goal of the project is to provide observational data that can be used to understand the character and physical processes associated with magnetic field generation and modulation in stars. Because we can spatially resolve magnetic structures only on the Sun, it must continue to provide the most fundamental information. However, we know that chromospheric emission, and therefore presumably magnetic field strengths, from stars correlates with rotation rate and properties of the convection zone. The chain of causality leading from fundamental stellar parameters to magnetic fields has not yet been elucidated definitively. But by observing other stars with different physical properties we can, in effect, study the physical consequences of perturbing variables (rotation rate, composition, age, mass, etc.) related to the physical mechanisms. For stars of earlier spectral type than the Sun we can study the effect of more rapid rotation, shallower (more quickly overturning) convection zones, and higher levels of acoustic flux on stellar activity. At much later spectral types, M5 or later, stars should be fully convective, and thus not possess a radiative/convective interface which is thought to be a probable location of stellar dynamos. By studying subgiants we may determine the evolutionary effect of a deepening convection zone. We have chosen not to study either binary systems or giants. We make this choice partly because we believe that a careful study of main sequence and subgiant stars will already strain our limited resources. In addition, although a study of binary systems and giants might well provide useful astrophysical insight, we believe that the additional physical processes active in such stars would render them less relevant to an eventual understanding of activity in solar-like stars. Thus our goals suggest a study of stars covering spectral types from mid-F to late M on the main sequence, and subgiants of types F and G. We desire that the stars be as bright as possible, with as much prior knowledge of their properties available as possible. The stars must be accessible from a latitude of 30° North. The Woolley, et al. (1970) "Catalogue of Stars Within Twenty Five Parsecs of the Sun" has been adopted as the primary source. In view of the above considerations, we applied the following criteria:
1)5 -25 0,
2) one of my, mR, mt< 8.5,
3) Mv > 2.0,
4) B - V > 0.2,
5) not a spectroscopic binary, which yielded a source list of about 750 stars, compared to a target list of under 400. Dropping troublesome binaries (secondary expected to contribute > 1% of light within 5 arc seconds) and stars without color indices further reduced this list to about 500 stars. In order to reduce the number of objects further we dropped all stars (except stars observed by O. C. Wilson) below the following series of line segments given by the (my, B -V) pairs: (5.0, 0.2), (5.5, 0.6), (7.0, 0.9), (9.5, 1.3), (9.5, 1.45), (13.0, 2.0). Wilson stars were dropped only in those cases in which serious blending from a companion was expected. Except for the retention of most Wilson (1978) survey stars falling outside the apparent magnitude limits described in the preceding paragraph, the list of 384 stars currently contained in the Catalog has not been biased as regards known magnetic or stellar structure properties. 4
Remaining steps were largely to make sure that our list contains: 1) an adequate number of subgiants, 2) an adequate number of subdwarfs, and 3) a few spectroscopic binaries with well known orbital parameters. To satisfy these requirements:
(1) An additional list of about 20 subgiants spanning mid-F to late-G spectral types, was added by searching The Bright Star Catalogue (1982) with the following criteria: 8 > -20°, Mv > 1.9, Mv < 3.0 + 2.89(B -V - 0.35), i > 0.025, my < 6.0, and 0.35 < B -V < 0.8. Three subgiant CH stars (see Sneden 1983), HD 4395, HD 89948 and HD 216219, were also added.
(2) The well documented subdwarfs HD 19445, HD 25329, HD 140283, and HD 201891, spanning spectral types of F6 to K2, were added to the list.
(3) The spectroscopic binaries HR 219A, HR 660, HR 4785, HR 5235, HR 5868, HR 6516, HR 9038, and GI 15A were added to provide calibration tests of detecting binarity over orbital periods of a few days to several years.
In addition all collaborators in the program were allowed to add one star to the list without regard to any formal criteria -- this explains, for example, the inclusion of the white dwarf 40 Eri B.
2. THE HAO-LOWELL-AFGL CATALOG
From the 384 stars in the catalog a subset of 138 stars were selected as candidates for the rotation mode of the program. These are located optimally for observation during the fall observing season. The remaining 246 stars, which are distributed more or less evenly over the remainder of the sky, serve as candidates for observation in the survey mode of the program. The catalog itself consists of two units. Each table contains two facing pages, the observational data on the left, and the catalog cross reference numbers on the right. As improved color information is received from others working in the field, it is possible that this Catalog may be updated and reissued at some future date. All catalog information is available on magnetic tape, which may be obtained upon request to: Kristine Fisher High Altitude Observatory P.O. Box 3000 Boulder, Colorado 80307 (303) 497-1522
In what follows we shall remark mainly on the sources of the data we have used; extensive discussions of methods, reduction procedures, errors, etc. can be found in the sources cited.
2.1. HAO # (High Altitude Observatory Number) The stars included in this catalog have been sorted by Right Ascension and HAO numbers have been assigned, incrementing by 10 to allow for the possibility of insertion of additional stars. The HAO number is therefore the principal index for all information relating to this star. The letter R or S following an HAO number designates the group, Rotation or Survey, into which the stars fall. 5
2.2. RA (Right Ascension) The right ascensions for stars included in this catalog were taken mainly from the SAO (Smithsonian Astrophysical Observatory) catalog; as a second choice we used the Catalogue of Stars Within Twenty-five Parsecs of the Sun by R. Woolley, et al. (1970). The position is recorded in hours, minutes, seconds, and tenths of seconds, with a precision of 0.1 seconds. Epoch 1950 was used throughout The catalog is organized by right ascension, with the Sun arbitrarily inserted with right ascension 00 00 00.0.
23. DEC (Declination) The declinations for stars included in this catalog were taken mainly from the SAO catalog, with the Woolley catalog as second choice. The position is recorded in degrees, minutes, and seconds of arc, with a precision of 1", at epoch 1950. The sun is arbitrarily assigned a declination of 00° 00' 00".
2.4. PMa (Proper Motion in Right Ascension) Annual proper motion in right ascension in seconds of time, Is , given to 0 0001. The primary source for these data was the SAO catalog, with the Woolley catalog as second choice. To convert to motion seen directly on the sky in seconds of arc per year gl must be multiplied by 15 cos 6.
2.5. PM8 (Proper Motion in Declination) Annual proper motion in declination in seconds of arc, Jtg, given to 0(001. The SAO catalog was used for the primary source of these data, and the Woolley catalog as second choice.
2.6. PAR (Parallax) Parallaxes, quoted to a precision of Y(I001, were taken primarily from the Woolley catalog (which, in turn, relied mainly on the Yale General Catalog of Trigonometric Stellar Parallaxes). The Bright Star Catalogue was used as a secondary source.
2.7. V (Visual Magnitude) Apparent visual magnitude on the standard Johnson-Morgan system, to a precision of 0.01. Our primary source for these data was the Bright Star Catalogue, and the Woolley catalog was used as the secondary source. We have not specifically flagged those cases where the magnitude (and colors) refer to the combined light of close or unresolved double stars, or are variable, because the photometric data given in this catalog are meant only for identification purposes and to provide estimates of relative exposure time in various bands.
2.8. B-V (Blue - Visual Color) The (B-V) color on the standard Johnson-Morgan system, to a precision of 0.01. The primary source for the data was the Bright Star Catalogue; the secondary source was the Woolley catalog.
2.9. U-B (Ultraviolet - Blue Color) The (U-B) color on the standard Johnson-Morgan system, to a precision of 0.01. The primary source for the data was the Bright Star Catalogue; the secondary source was the Woolley catalog. 6
2.10. R-I (Red - Infrared Color) Our primary source for (R-I) colors was the Bright Star Catalogue which includes colors from three non-identical systems (Johnson, Eggen, and Cousins - see the Bright Star Catalogue introduction); for the reasons given in § 2.7 above, we have not attempted to differentiate among these systems in this catalog. As secondary sources we used the Gliese catalog (1969), and the extensive computer-readable multicolor photometric catalog of Morel and Magnenat (1978).
2.11. I (Infrared Magnitude) Infrared magnitudes on the standard Johnson IJKLMNH system, to a precision of 0.01, taken from the Morel and Magnenat (1978) photoelectric photometry catalog.
2.12. SPEC (Spectral Type) The spectral types listed in this catalog were taken from the Woolley catalog (1970), the Bright Star Catalogue (1983), and the Gliese catalog (1969), in that order of preference. In principle all three sources use the Morgan-Keenan System, but in practice there is a large range in the quality of the classifications in all of them. In fact most are quite rough. The data appear in the form of a luminosity class indicator, spectral type, and note. For luminosity class we use the code: 3 = giant, 4 = subgiant, 5 = dwarf, 6 = subdwarf, and 37 = white dwarf. As notes we use e to indicate emission (often Ha) and p to indicate a peculiar spectrum (in some cases an extreme metal-poor star).
2.13. RV (Radial Velocity) Radial velocities in km/s, to a precision of 0.1 km/s, were drawn from the Woolley catalog, the Bright Star Catalogue, and the Gliese catalog, in that order of preference. Most of these sources rely, in turn, on R. E. Wilson's radial velocity catalog (1953).
2.14. HK (CaII H and K Flux) The table entry HK gives the flux index, S (defined in Vaughn, Preston, and Wilson 1978), proportional to the total equivalent width of the emission reversals and underlying residual photospheric light in one Angstrom bands centered at H and K. The compilation of data for a large number of stars is summarized in Vaughn and Preston (1980). An updated version of the data was supplied to us by Dr. Sallie L. Baliunas. Typical precisions are about 3%. When available, the more precise values from Noyes, et al. (1984) were adopted.
2.15. W # (Woolley Catalog Number) The table entry W# gives the catalog number in the Woolley catalog (1970). Numbers from the Gliese catalog (1969) contain a decimal point and fall between existing Woolley numbers. The letter notations (A, B, etc.) designate components.
2.16. BS # (Bright Star Catalogue Number) The catalog entry BS# gives the number used in the Bright Star Catalogue (Hoffleit 1982).
2.17. HD # (Henry Draper Catalogue Number) Catalog number from the Henry Draper Catalogue or its Extension. 7
2.18. SAO # (Smithsonian Astrophysical Observatory Catalog Number) The entry SAO # gives the Smithsonian Astrophysical Observatory Catalog number. For our catalog this number was obtained by cross-referencing HD numbers in the HD-SAO-DM-Cross Index, NASA TM79564 (Nagy, 1978).
2.19. BD # (Bonner Durchmusterung Number) This entry gives the number from the Bonner Durchmusterung for stars in zones north of -23°, and from the Cordoba Durchmusterung for stars in the zones -23° to -52°. This number was obtained principally from the HD-SAO-DM-Cross Index, NASA TM79564, by (Nagy, 1978). It was verified in the Gliese catalog (1969), the Bright Star Catalogue (Hoffleit 1982), and the SAO Catalog (1966).
2.20. FIND CHART (Finding Chart) This entry gives a finding chart number for identification fields (18' on a side) contained in the Lowell Observatory Bulletin (Giclas, et al. 1959-1969).
2.21. BIN (Binary) Single letter confirmation of binary status, and designation of type of binary. Y Binary, but type unknown N Not a binary star S Spectroscopic 0 Optical A Astrometric C Common proper motion V Visual E Eclipsing 8
2.22. ABBREVIATIONS USED
AC Astrographic Catalogue ADS Aitken Double Star catalog number a separation ±xx.x" in arc sec(") and minute(') a sini projected separation between components (B) Bidelman 1954 C number of components CN constellation name cp companion cpm common proper motion d days Am change in magnitude xx.x G group HK HK flux I infrared K half amplitude of the radial velocity curve of a SB (km/s) km/s kilometers per second LT Luyten catalog number MK Morgan-Keenan system N name m sini3 stellar mass times cube of orbital inclination OW Olin Wilson star P period x.x y=year d=days P rotation period RPrt radial velocity SB spectroscopic binary SD subdwarf SG subgiant V variable V visual magnitude, i.e. 12.0V V? possibly variable v sini projected rotation velocity Vys Vyssotsky catalog number W# Woolley catalog number y years ~~" ~ arc seconds ~~' ~ arc minutes
3. ACKNOWLEDGEMENTS
We wish to give sincere thanks to Dr. Sallie L. Baliunas for assistance with the compilations of Cal H and K fluxes, and to Louise Beierle for the immense amount of work she did in entering and checking the data contained in this catalog. 9
4. REFERENCES
Bidelman, W.P., Astrophysical Journal Supplement, 1, 175, 1954.
Cannon, A.J. and Pickering, E.C., The Henry Draper Catalogue, Annals of the Astronomical Observatory of Harvard College, Vols. 91-99, 1918-1924. Cannon, A.J., The Henry Draper Extension, Annals of the Astronomical Observatory of Harvard College, Vol. 100, 1925-36.
Cannon, A.J., The Henry Draper Charts of Stellar Spectra, Annals of the Astronomical Observatory of Harvard College, Vol. 105, 1, 1937.
Cannon, A.J. and Mayall, M.W., The Henry Draper Extension, Annals of the Astronomical Observatory of Harvard College, Vol. 112, 1949. Giclas, H.L., Slaughter, C.D. and Burnham, R., Lowell Obs. Bull., No. 102, 1959. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 112, 1961. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 120, 1963. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 122, 1964. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 124, 1964. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 129, 1965. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 132, 1966. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 136, 1966. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 138, 1967. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 140, 1967. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 144, 1968. Giclas, H.L., Burnham, R., and Thomas, N.G., Lowell Obs. Bull., No. 150, 1969. Gliese, W., Catalog of Nearby Stars, Verlag G. Braun, Karlsruhe, 1969. Hoffleit, D., The Bright Star Catalogue (Fourth Revised Edition), Yale University Observatory, New Haven, Conn., 1982.
Hoffleit, D., Saladyga, M., and Wlasuk, P., A Supplement to the Bright Star Catalogue, Yale University Observatory, New Haven, Conn., 1983. Morel, M., and Magnenat, P., UBVRIJKLMNH Photoelectric Photometric Catalogue, Astronomy and Astrophysics Supplement, 34, 447, 1978.
Nagy, T.A., and Mead, J., HD - SAO - DM - Cross Index, NASA TM79564, Goddard Space Flight Center, Greenbelt, MD., 1978. 10
Noyes, R.W., Hartmann, L.W., Baliunas, S.L., Duncan, D.K., and Vaughan, A.H., Rotation, Convection, and Magnetic Activity in Lower Main-Sequence Stars, Ap.J., 279 763, 1984.
The Smithsonian Astrophysical Observatory Catalog: Positions and Proper Motions of 258,997 Stars for the Epoch and Equinox of 1950.0, Smithsonian Institution, Washington, D.C., 1966.
Sneden, C., Carbon and Oxygen in the Subgiant CH Stars, Pub. Ast. Soc. Pacific, 95, 745, 1983.
Vaughan, A.H., and Preston, G.W., A Survey of Chromospheric CAII H and K Emission in Field Stars of the Solar Neighborhood, Pub. Astr. Soc. Pacific, 92, 385, 1980.
Vaughan, A.H., Preston, G.W., and Wilson, O.C., Flux Measurements of Call H and K Emission, Pub. Astr. Soc. Pacific, 90, 267, 1978.
Wilson, O.W., Chromospheric Variations in Main-Sequence Stars, Ap.J., 226, 379, 1978.
Woolley, R., Epps, E.A., Penston, M.J. and Pocock, S.B., Catalogue of Stars Within Twenty-five Parsecs of the Sun, Royal Observatory Annals, Number 5, Herstmonceux, Royal Greenwich Observatory, 1970. 11
5. CATALOG 12
SOLAR STELLAR SPECTROPHOTOMETER CATALOG High Altitude Observatory - NCAR - Left Page
HAO # RA DEC PMa PM8 PAR V B-V U-B R-I I
0 R 00 00 00.0 00 00 00 0.000 0.000 0.000 -26.5 0.66 0.10 10 R 00 02 32.0 +45 30 36 +0.083 -0.15 0.094 9.89 1.50 1.18 - 20 R 00 04 00.7 +28 44 44 +0.0289 -0.177 0.069 6.13 0.75 0.33 - 30 R 00 08 43.0 -15 44 33 -0.0056 -0.264 0.066 4.89 0.49 -.03 - 40 R 00 14 26.0 +40 40 12 +0.049 +0.09 0.063 9.00 1.37 1.19 0.61
50 R 00 15 30.9 +43 44 22 +0.2653 +0.404 0.282 8.08 1.56 1.24 0.88 5.52 60 R 00 15 34.0 +43 44 42 +0.264 +0.40 0.282 11.04 1.80 1.40 1.22 7.65 70 R 00 20 18.0 -12 29 15 +0.0266 +0.065 0.049 6.39 0.66 0.24 -- 80 R 00 25 44.7 +09 54 58 +0.0022 -0.203 0.033 6.04 0.43 -.06 --- 90 R 00 32 58.7 -00 46 48 +0.0089 -0.058 - 5.93 0.44 -.02 -
100 R 00 34 46.7 -25 02 32 +0.1022 -0.007 0.074 5.57 0.72 0.24 0.27 - 110 R 00 36 45.4 +20 58 52 -0.0331 -0.366 0.100 5.87 0.85 0.57 0.39 4.82 120 R 00 38 01.8 -24 04 27 +0.0469 -0.328 0.042 6.14 0.70 0.21 -- 130 R 00 38 04.3 +39 55 20 +0.0301 -0.666 0.072 7.35 0.93 0.71 140 R 00 40 52.0 +33 34 36 -0.017 -0.37 0.058 8.70 1.13 1.09 0.44
150 R 00 43 43.0 -11 43 30 -0.0076 -0.056 -- 160 R 00 45 45.5 +05 01 26 +0.0506 -1.142 0.144 5.75 0.88 0.59 0.47 4.52 170 R 00 46 03.0 +57 33 06 +0.137 -0.52 0.172 7.51 1.39 1.03 0.59 - 180 R 00 46 03.6 +57 33 03 +0.1368 -0.521 0.172 3.44 0.57 0.01 0.36 - 190 R 0047 37.3 -10 54 48 -0.0156 -0.223 0.064 5.19 0.50 -.02 0.28 4.46
200 R 00 49 04.2 -23 10 41 +0.0451 -0.278 0.068 8.93 1.29 2.33 -- 210 R 00 50 04.0 +60 51 01 -0.0098 +0.178 0.064 4.82 0.53 0.12 0.30 4.04 220 R 00 59 27.0 +62 04 30 +0.106 +0.09 0.109 9.57 1.50 1.21 0.89 - 230 R 01 03 44.0 +63 40 12 +0.2280 +0.280 0.072 8.98 1.30 1.21 0.56 - 240 R 01 04 55.7 +54 40 33 +0.3947 -1.575 0.127 5.17 0.69 0.09 0.42 4.13
250 R 01 04 55.7 +22 41 42 +0.0073 -0.482 0.043 8.40 1.12 1.06 -- 260 R 01 07 27.8 +41 48 58 -0.0122 -0.037 5.65 0.60 ---- 270 R 01 11 52.8 -08 11 28 +0.0082 +0.277 0.051 5.13 0.46 -.05 - 280 R 01 17 50.4 +76 26 57 -0.0035 -0.031 0.042 7.11 0.82 0.45 ---- - 290 R 01 24 39.2 +45 08 58 +0.0328 -0.100 0.030 4.83 0.42 0.00 0.23 4.19
300 R 01 30 52.9 -24 25 55 +0.0215 -0.152 0.070 6.97 0.76 1.86 0.38 - 310 R 01 31 11.8 -07 16 49 +0.0118 -0.077 - 5.76 0.64 0.21 ---- - 320 R 01 33 51.1 +41 09 22 -0.0153 -0.379 0.062 4.09 0.54 0.06 0.29 3.35 330 R 01 38 43.8 +42 21 49 +0.0730 -0.147 0.087 4.95 0.62 0.12 0.33 - 340 R 01 39 46.6 +20 01 34 -0.0209 -0.668 0.134 5.24 0.84 0.49 0.43 4.12 13
SOLAR STELLAR SPECTROPHOTOMETER CATALOG High Altitude Observatory - NCAR - Right Page
HAO # SPEC RV HK W# BS# HD# SAO # BD # FIND CHART BIN
O R 5G2 0.0 SUN ------N 10 R 5M2 e +0.2 2.138 2 ------..--.. +44 4548 129G171-39 C 20 R 5 KOe - 8.2 0.486 5 8 166 73743 +28 4704 Y 30 R 5 F6 +14.8 -- 10 33 693 147133 -16 0017 40 R 5 MO + 2.2 2.039 14 ------...-.- +40 0045 129G171-44
50 R 5 M1 +13.6 -- 15A ---- 1326 36248 +43 0044 129G171-47 S 60 R 5 M6 e +20.7 1.512 15B ------G171-48 70 R 5 G2 - 6.8 0.360 9012 88 1835 147237 -13 0060 0 80 R 5 F6 -10.0 0.170 --- 107 2454 109224 +09 0047 90 R 4 F5 + 6.0 0.215 --- 143 3229 128843 -01 0068 ------
100 R 5 G5 +16.5 0.182 25A 159 3443 166418 -25 0225 S 110 R 5KO -34.2 0.185 27 166 3651 74175 +20 0085 Y 120 R 5 G3 -52.9 0.158 9019 173 3795 166475 -24 0263 130 R 5 K2 e -63.2 0.229 28 ---- 3765 54074 +39 0154 G132-15 140 R 5 K5 -32.9 0.617 30 ------... +33 0099 G069-15
150 R 4 G5 p . 4395 147438 -12 0132 160 R 5 K2 -12.6 0.230 33 222 4628 109471 +04 0123 Y 170 R 5 MO +12.8 1.246 34B S 180 R 5 GO + 9.4 0.159 34A 219 4614 21732 +57 0150 S 190 R 5 F8 + 7.7 37 235 4813 147470 -11 0153
200R 5 K4e +15.5 40 ---- 4967 166631 -23 0332 210 R 5 F8 +20.7 0.146 41 244 5015 11444 +60 0124 S 220 R 5 K5 e - 5.1 2.385 49 ------+61 0195 G243-52 C 230 R 5 K7 - 3.4 1.072 52 -----. +63 0137 G243-60 240 R 6 G5 p -97.2 0.168 53 321 6582 22024 +54 0223 A
250 R 5 K4 - 3.4 0.587 9040A ---- 6660 74504 +22 0176 G34-2 0 260 R 5 F8 -11.0 0.190 53.4 340 6920 36984 +41 0219 270 R 5 F5 +22.0 9045A 366 7439 129193 -08 0216 C 280 R 5 KO -22.7 0.222 9054 ---- 7924 4386 +75 0058 290 R 4F5 p +11.0 0.237 ----- 417 8799 37228 +44 0307 . ------0
300 R 5 G8 -0.1 59 ---- 9540 167134 -24 0658 Y 310R 4G2 -15.0 0.145 59.2 448 9562 129371 -07 0256 320 R 5 F8 -28.1 0.153 61 458 9826 37362 +40 0332 S 330 R 5G2 + 4.0 0.154 67 483 10307 37434 +41 0328 A 340 R 5 K1 -33.7 0.210 68 493 10476 74883 +19 0279 Y 14
HAO # RA DEC PMa PM8 PAR V B-V U-B R-I I
350 R 01 40 11.7 +63 34 50 -0.0611 -0.567 0.075 8.40 1.22 1.14 0.48 360 R 01 41 44.7 -16 12 01 -0.1194 +0.858 0.277 3.50 0.72 0.21 0.47 2.41 370 R 01 42 11.6 +19 50 03 -0.0029 -0.105 0.056 6.27 0.75 0.23 380 R 01 44 06.4 +63 36 24 +0.0876 -0.246 0.114 5.63 0.81 0.40 0.39 4.60 390 R 01 50 25.3 -22 40 51 +0.0598 +0.007 0.083 8.70 1.41 ------
400 R 01 54 43.0 -10 28 57 -0.0257 -0.228 0.050 6.41 0.82 0.48 0.29 410 R 01 57 32.9 +02 51 32 +0.0152 -0.246 0.034 5.88 0.62 0.19 - 420 R 02 02 37.0 -17 51 06 +0.0900 -0.160 0.114 10.18 1.53 1.16 1.02 7.34 430 R 02 08 42.4 +08 20 12 -0.0095 -0.108 0.034 5.63 0.56 0.14 -- 440 R 02 11 35.4 +67 26 39 +0.0932 -0.304 0.045 7.09 0.90 0.74 --
450 R 02 13 59.6 +33 59 48 +0.0928 -0.237 0.093 4.87 0.61 0.02 0.24 460 R 02 15 25.4 +01 31 20 +0.0241 +0.375 0.038 5.58 0.60 0.10 - 470 R 02 18 57.0 +47 39 06 +0.0220 +0.040 0.095 9.41 1.49 1.18 0.78 - 480 R 02 20 15.2 -24 02 34 +0.0144 -0.056 0.076 5.20 0.60 0.12 0.36 4.30 490 R 02 29 42.9 -15 27 47 -0.0053 -0.117 0.035 4.75 0.45 -.02 0.27 -
500 R 02 33 20.1 +06 38 58 +0.1208 +1.461 0.144 5.82 0.98 0.81 0.53 510 R 02 37 46.3 -09 39 57 -0.0106 -0.084 5.78 0.52 0.00 - 520 R 02 40 30.4 +19 13 04 +0.0299 -0.012 0.055 8.27 1.07 0.95 - 530 R 02 40 46.3 +49 01 06 +0.0342 -0.083 0.079 4.12 0.49 0.00 0.30 3.37 540 R 02 42 46.1 -18 46 59 +0.0229 +0.042 0.073 4.47 0.48 0.00 0.27 3.76
550 R 02 47 49.4 +15 30 34 +0.0235 -0.395 0.059 8.90 1.27 ------560 R 02 50 07.4 -12 58 16 +0.0266 -0.172 0.127 6.04 0.87 0.56 0.45 4.88 570 R 02 53 36.5 +17 49 30 +0.0193 -0.207 0.038 5.63 0.43 -.02 -- 580 R 03 03 50.1 +01 47 09 +0.0258 -0.884 0.063 9.09 1.36 1.22 0.64 - 590 R 03 05 26.7 +49 25 27 +0.1295 -0.078 0.086 4.05 0.59 0.12 0.29
600 R 03 05 28.7 +26 09 08 -0.0149 -0.795 -- 8.06 0.46 -.24 ---- 7.27 610 R 03 10 13.2 -01 22 55 +0.0129 -0.063 0.049 5.06 0.57 0.12 -- 620 R 03 16 44.1 +03 11 17 +0.0178 +0.098 0.107 4.83 0.68 0.19 0.36 3.91 630 R 03 22 31.6 -05 31 43 -0.0167 -0.775 0.065 7.85 1.16 1.16 -- 640 R 03 25 35.7 -19 58 52 +0.0362 +0.334 0.071 8.38 1.34 1.18 0.57 -
650 R 03 30 34.4 -09 37 35 -0.0662 +0.019 0.302 3.73 0.88 0.59 0.47 2.53 660R 03 31 17.2 +17 40 13 +0.0063 -0.313 0.022 6.17 0.89 0.54 - 670 R 03 34 19.1 +00 14 40 -0.0157 -0.481 0.061 4.28 0.58 0.07 0.32 3.47 680 R 03 38 33.6 +03 27 18 -0.0019 -0.229 0.054 9.65 1.43 ---- 0.60 - 690 R 03 40 51.0 -09 55 53 -0.0067 +0.746 0.111 3.54 0.92 0.69 0.50 2.32
700 R 03 43 04.2 +68 30 57 +0.0200 +0.292 0.052 9.26 1.30 1.18 ---- - 710 R 03 44 41.7 -23 23 47 -0.0118 -0.527 0.057 4.23 0.42 0.00 0.22 3.62 720 R 03 52 08.6 -06 58 46 -0.0015 +0.531 0.076 9.04 1.36 1.21 0.62 - 730 R 03 54 48.9 +76 01 34 +0.0968 -0.520- 0.050 8.26 1.15 1.04 ---- - 740 R 03 54 56.8 -01 18 03 -0.0125 -0.158 0.102 8.06 1.12 1.01 0.49 15
HAO # SPEC RV HK W # BS # HD# SAO # BD # FIND CHART BIN
350 R 5 K5 -48.3 0.981 69 10436 11943 +63 0229 G244-33 360 R 5 G8 p -16.2 0.172 71 509 10700 147986 -16 0295 Y 370 R 5 G4 -43.5 0.137 72 508 10697 92611 +19 0282 380 R 5 K + 1.8 0.317 75 511 10780 11983 +63 0238 A 390 R 5 M1e +25.9 ----- 79 - 11507 167374 -23 0693
400 R 4G5 -6.8 ----- 9063 - 11964 148123 -10 0403 0 410 R 4G2p -17.0 0.170 83.2 582 12235 110266 +02 0311 420 R 5 MO -35.0 - 8-84 ...... -18 0359 430 R 4 GO -18.0 0.130 --- 635 13421 110390 +07 0347 440 R 5 K2 -13.7 0.333 90 - 13579 12190 + 67 0191 G244-56 0
450 R 5 GO - 6.0 0.232 - 660 13974 55420 +33 0395 -..-....-. S 460 R 4 G.5p +27.0 672 14214 110456 +01 0410 470 R 5 M2 e -34.6 -- 96 ------.....-- -.-- +47 0612 G173-53 480 R 5G1 +18.4 ----- 97 695 14802 167736 -24 1038 ------490 R 4 F4 p -29.0 -- 740 15798 148445 -15 0449 ------
500 R 5 K3 p +23.4 0.230 105A 753 16160 110636 +06 0398 G073-70 C 510 R 5F6 -4.0 0.215 --- 784 16673 130047 -10 0525 520 R 5 K4 +32.9 ----- 106 - 16909 93072 +18 0339 102G004-35 530 R 5 F7 +25.0 0.159 107A 799 16895 38288 +48 0746 0 540 R 5 F6 +25.6 -- 111 818 17206 148584 -19 0518 ------r S
550 R 5 K6 -25.0 --- 114 - 17660 93138 +15 0395 102G004-43 560 R 5 KO +18.8 0.700 117 857 17925 148647 -13 0544 570 R 5F6 +15.0 0.170 - 869 18256 93195 +17 0458 S 580 R 5 MO -21.9 1.465 123 - 19305 110970 +01 0543 112G076-58 590 R 5 G4 +50.0 0.152 124 937 19373 38597 +49 0857 Y
600 R 5F2p -- 19445 75749 +25 0495 610 R 5 F8 +18.3 ----- 128A 962 19994 130355 -01 0457 0 620 R 5 G5 e +19.3 0.345 137 996 20630 111120 +02 0518 Y 630 R 5 K5 -11.8 ----- 141 - 21197 130471 -05 0642 112G077-49 640 R 5K7 +31.3 ----- 142 - 21531 148971 -20 0643
650 R 5 K2e +15.4 0.510 144 1084 22049 130564 -09 0697 A 660 R 4 K1 +11.0 0.135 - 1085 22072 93494 +17 0575 670 R 5 F8 +27.9 ----- 147 1101 22484 111292 -00 0572 C 680 R 5 MOp + 0.9 1.466 148 ...... --- 111352 +03 0515 112G080-17 690 R 4 KOe - 6.4 0.137 150 1136 23249 130686 -10 0728
700 R 5 MO - 4.7 0.778 153A - 23189 12903 +68 0278 G221-23 0 710 R 5 F3 + 6.5 -- 155 1173 23754 168827 -23 1565 720 R 5 MO +58.3 -- 156 ------.-- 130811 -07 0699 122G160-35 730 R 5 K4 +20.0 0.848 9139 24451 5056 +75 0154 740 R 5 K5 e + 5.7 ----- 157A 24916 130840 -01 0565 0 16
HAO # RA DEC PMa PMS PAR V B-V U-B R-I I
750 R 03 59 53.2 +35 09 17 +0.1420 -1.346 0.052 8.52 0.88 0.36 760 R 04 00 02.8 -00 24 12 +0.0097 -0.248 0.055 5.38 0.50 0.00 770 R 04 02 22.4 +21 52 32 +0.0122 -0.133 0.069 5.90 0.62 0.12 780 R 04 05 16.2 +37 54 39 +0.0139 -0.198 0.046 5.51 0.46 -.03 790 R 04 12 45.9 +06 04 38 -0.0073 -0.105 6.93 0.70 0.22
800 R 04 12 49.2 +06 03 51 -0.0042 -0.114 - 6.31 0.59 0.05 810 R 04 12 58.2 -07 43 46 -0.1501 -3.420 0.205 4.43 0.82 0.45 0.45 3.29 820 R 04 13 03.7 -07 44 09 -0.1469 -3.440 0.205 9.53 0.03 -.68 0.83 830 R 04 13 04.0 -07 44 06 -0.1460 -3.420 0.205 11.16 1.68 840 R 04 26 02.0 +21 48 40 -0.0045 +0.183 0.078 8.27 1.35 1.22 0.62
850 R 04 33 43.3 +52 48 01 +0.0346 -0.460 0.093 8.61 1.41 1.14 0.65 860 R 04 37 01.6 -14 27 17 +0.0080 -0.127 0.007 5.45 1.06 870 R 04 38 22.0 +20 48 34 -0.0166 -0.260 0.082 8.02 1.18 880 R 04 38 26.0 +38 11 11 +0.0201 -0.096 0.022 5.99 0.57 0.06 890 R 04 39 58.0 +18 52 54 +0.0500 -1.050 0.097 9.94 1.54 1.18 0.96
900 R 04 45 21.5 -17 01 29 +0.0088 +0.171 0.077 5.51 0.63 0.12 0.34 4.62 910 R 04 46 07.9 -05 45 26 +0.0201 -0.241 0.038 5.78 0.62 0.20 920 R 04 57 43.5 +14 18 36 +0.0033 +0.054 6.76 930 R 04 58 19.9 -05 48 38 +0.0369 -1.091 0.109 6.22 1.06 1.02 0.49 4.87 940 R 05 01 15.0 -23 19 19 +0.0214 +0.142 0.058 9.29 1.28 1.23 0.64
950 R 05 06 14.8 -04 31 11 +0.0026 +0.018 0.048 5.12 0.44 -.05 960 R 05 06 59.2 +46 54 09 +0.0056 -0.146 0.027 5.68 0.42 0.02 970 R 05 08 48.0 -02 33 03 +0.0045 +0.009 5.90 0.46 0.04 980 R 05 14 16.6 +79 10 43 -0.0285 +0.160 0.053 5.05 0.47 -.13 990 R 05 15 37.2 +40 03 25 +0.0456 -0.661 0.067 4.71 0.63 0.12 0.32 3.86
1000R 05 16 40.2 -03 07 36 +0.0482 +0.127 0.074 7.75 1.05 0.85 1010R 05 20 40.3 +17 16 42 +0.0187 -0.002 0.057 7.97 1.09 1.00 0.43 1020R 05 21 30.2 +17 20 20 +0.0172 -0.008 0.064 4.99 0.53 -.07 1030R 05 25 57.3 -03 31 42 -0.0219 -0.797 0.072 7.63 1.10 1.19 0.44 1040R 05 28 55.3 -03 41 04 +0.0512 -2.099 0.170 7.97 1.47 1.21 0.85 5.39
1050R 05 33 44.0 +11 17 54 -0.0010 -0.050 0.082 8.82 1.38 1.18 0.65 1060R 05 37 16.8 +53 27 48 +0.0008 -0.518 0.091 6.23 0.84 0.51 0.43 5.11 1070R 05 37 27.1 +53 28 20 +0.0022 -0.494 0.117 9.78 1.49 1.15 0.82 1080R 05 41 06.0 +62 13 42 +0.0370 -0.790 0.079 9.02 1.40 1.23 0.63 1090R 05 42 21.4 -22 26 13 -0.0225 -0.355 0.123 6.15 0.94 0.74 0.35
11 OOR 05 42 22.7 -22 27 48 -0.0212 -0.373 0.123 3.60 0.47 0.00 0.26 2.89 1110R 05 44 00.1 +01 09 08 -0.0051 -0.148 0.027 5.95 0.78 0.42 1120R 05 51 25.2 +20 16 07 -0.0133 -0.086 0.101 4.41 0.59 0.07 0.31 3.59 1130R 05 54 07.6 -14 10 32 -0.0034 +0.136 0.065 3.71 0.33 0.01 0.16 3.23 1140R 06 03 48.6 +15 32 59 -0.0079 -0.109 0.065 6.76 0.81 0.42 ------17
HAO # SPEC RV HK W # BS # HD # SAO # BD # FIND CHART BIN - - I------BIN I
750 R 5 Kl p -30.0 0.189 158 - 25329 56928 +34 0796 760 R 5 F6 +17.5 159 1249 25457 130893 -00 0632 770 R 5 G1 +25.6 0.281 160 1262 25680 76438 +21 0587 Y 780 R 5 F7 +24.8 0.275 9145 1278 25998 57006 +37 0882 C 790 R 4 G5 - 8.0 0.385 1321 26913 111695 +05 0613 C
800 R 4 GO - 8.0 0.285 -- 1322 26923 111698 +05 0614 C 810 R 5 K e -42.4 0.205 166A 1325 26965 131063 -07 0780 G160-60 0 820 R 7 A p -21.0 166B - 26976 131065 -07 0781 122G160-60 0 830 R 5 M4 e -45.0 6.588 166C 0 840 R 5 M1 e -33.6 1.359 169 28343 76626 +21 0652
850 R 5 K8 e +36.2 1.909 172 - 232979 24722 +52 0857 129G175-42 860 R 4 K p +56.0 1487 29613 149797 -14 0936 870 R 5 K3 e + 8.0 2.244 174 - 29697 76708 +20 0802 G008-51 880 R 5 GO +47.0 0.135 1489 29645 57377 +37 0954 890 R 5 M3 e +29.0 1.285 176 - 285968 -....- +18 0683 102G008-55
900 R 5 G1 +16.8 0.285 177 1532 30495 149888 -17 0954 910 R 5 F8 p +79.0 .. 177.1 1536 30562 131504 -05 1044 Y 920 R 4-5G2p -16.0 ----- 182.1 - 31966 94253 +14 0804 930 R 5 K3 +27.0 0.300 183 1614 32147 131688 -05 1123 S 940 R 5 MO 124. 186 170021 -23 2363
950 R 5 F5 + 9.4 -- 9176 1673 33256 131813 -04 1056 960 R 5 F5 p +33.0 1668 33167 40077 +46 0970 970 R 5 F5 +31.0 0.210 ----- 1687 33608 131852 -02 1165 980 R 5 F6 - 9.9 0.149 196 1686 33564 5496 +79 0169 0 990 R 5 GO +65.7 0.149 197 1729 34411 40233 +39 1248 0
1000R 5 K3 +85.2 -- 200A 34673 131977 -03 1061 G084-45 0 1010R 5 K5 +37.4 1.013 201 ---- 35171 94513 +17 0917 112G085-68 C 1020R 5 F8 e +36.5 0.308 202 1780 35296 94526 +17 0920 0 1030R 5 K5 -58.2 204 36003 132145 -03 1110 112G099-12 1040R 5 M1 e +10.9 205 - 36395 132211 -03 1123 112G099-15
1050R 5 MO +23.3 2.625 208 ------+11 0878 1060R 5Kl e +0.9 0.478 211 1925 37394 25319 +53 0934 C 1070R 5 M2 + 0.5 2.198 212 25321 +53 0935 136G191-51 C 1080R 5 MOep -16.5 -- 215 ------+62 0780 1090R 5 K2 -10.1 -- 216B 1982 38392 170757 -22 1210 ------C
1100R 5 F6 - 9.7 ----- 216A 1983 38393 170759 -22 1211 C 11OR 5 G4 p +29.0 1988 38529 113119 +01 1126 1120R 5 GO -13.5 0.300 222 2047 39587 77705 +20 1162 S 1130R 4 F0 - 1.6 ----- 225 2085 40136 150957 -14 1286 1140R 5 KO e -11.7 0.456 227 41593 95235 +15 1065 18
HAO # RA DEC PMa PMS PAR V B-V U-B R-I I
1150R 06 08 28.1 -21 50 36 -0.0094 -0.725 0.174 8.14 1.49 1.23 0.82 1160R 06 13 38.1 +12 17 16 +0.0055 +0.185 0.042 5.04 0.42 -.02 -- -- 1170R 06 14 37.1 +05 07 02 -0.0147 +0.158 0.050 5.71 0.61 0.10 1180R 06 22 43.0 -00 54 50 +0.0147 -0.225 0.027 5.87 0.56 0.08 0.20 1190S 06 34 19.0 +17 36 12 -0.0550 +0.330 0.104 9.63 1.50 1.18 0.74 -
1200S 06 38 11.9 +24 00 34 +0.0150 -0.275 0.086 8.15 1.03 0.91 0.38 1210S 0642 29.0 +12 57 04 -0.0079 -0.194 0.055 3.36 0.43 0.06 0.23 2.74 1220S 06 43 08.2 +43 37 46 -0.0002 +0.164 0.068 5.25 0.56 0.05 -- 1230S 06 45 26.7 +60 23 14 +0.0321 +0.402 0.084 8.58 1.20 1.14 0.48 - 1240S 06 47 49.0 +47 26 12 -0.0240 -0.720 0.075 9.00 1.23 1.16 0.50
1250S 06 49 52.0 -05 06 43 -0.0365 -0.004 0.104 6.59 1.06 0.95 0.38 1260S 06 51 35.0 +33 20 18 -0.0580 -0.420 0.168 9.90 1.60 1.20 1.09 1270S 06 51 49.0 +13 14 36 +0.0054 -0.086 0.042 7.68 0.72 0.20 - 1280S 06 52 14.2 +25 26 24 -0.0030 +0.020 0.053 5.73 0.57 0.00 0.01 1290S 06 59 10.6 -25 52 37 +0.0149 +0.038 0.068 6.71 0.90 2.01 0.30
1300S 07 06 39.0 +38 37 30 -0.0400 -0.920 0.169 11.47 1.71 1.19 1.39 1310S 07 12 07.6 +47 19 51 +0.0032 -0.183 0.037 5.58 0.58 0.03 - 1320S 07 24 23.4 +31 58 02 -0.0011 -0.002 0.042 7.73 0.94 0.67 - 1330S 07 24 43.0 +05 22 42 +0.0400 -3.690 0.270 9.82 1.56 1.12 1.19 - 1340S 07 31 54.7 -22 11 13 -0.0033 +0.039 0.053 4.45 0.51 0.06 0.27 3.67
1350S 07 34 47.5 -03 59 53 -0.0049 +0.014 0.028 5.13 0.44 0.12 -- 1360S 07 36 41.1 +05 2117 -0.0473 -1.029 0.292 0.38 0.42 0.02 0.23 -.28 1370S 07 36 48.0 +02 18 12 -0.0040 -0.180 0.077 9.66 1.38 1.30 0.71 - 1380S 07 37 29.1 -03 28 39 +0.0048 -0.290 0.085 7.20 0.96 0.73 0.32 1390S 07 37 33.0 -03 29 00 +0.0050 -0.288 0.085 8.94 1.33 1.24 0.57 -
1400S 08 04 49.4 +21 43 42 +0.0015 -0.074 0.034 5.30 0.63 0.21 -- 1410S 08 16 01.5 -12 27 41 +0.0181 -0.983 0.079 5.98 0.76 0.33 0.38 1420S 08 17 01.8 +27 22 52 -0.0012 -0.382 0.063 5.14 0.47 -.06 -- 1430S 08 31 55.0 +67 28 06 -0.1830 +0.000 0.078 9.30 1.42 1.23 0.71 - 1440S 08 34 46.7 +65 11 45 -0.0039 +0.086 0.064 5.64 0.62 0.07 0.33 4.79
1450S 08 47 26.1 +33 28 24 -0.0053 -0.085 - 6.25 0.49 0.01 -- 1460S 08 47 34.0 +66 19 06 +0.0150 +0.100 0.076 9.29 1.33 1.22 0.57 1470S 08 49 37.4 +28 31 23 -0.0366 -0.239 0.074 5.95 0.87 0.63 0.40 1480S 08 50 44.6 +70 59 26 -0.2770 -0.385 0.091 8.04 1.39 1.24 0.62 1490S 08 51 50.1 -05 14 39 -0.0282 +0.026 0.085 6.00 0.67 0.22 0.21
1500S 08 56 23.1 -15 5627 +0.0162 +0.214 0.028 5.86 0.53 0.08 0.23 1510S 09 05 47.3 +34 05 12 -0.0150 -0.124 - 5.93 0.60 0.04 -- -- 1520S 09 10 58.8 +52 54 07 -0.1737 -0.587 0.166 7.62 1.38 1.20 0.68 - 1530S 09 11 00.9 +52 54 10 -0.1712 -0.679 0.166 7.72 1.38 1.20 ---- 1540S 09 21 35.2 +76 09 07 -0.1007 -0.103 0.058 9.03 1.19 1.18 0.46 - 19
HAO # SPEC RV HK W# BS # HD # SAO # BD # FIND CHART BIN
1150R 5 M1 e + 3.0 -- 229 ---- 42581 171334 -21 1377 1160R 4 F5 + 8.7 0.226 9207 2241 43386 95476 +12 1084 0 1170R 5 GO +12.8 0.158 9208A 2251 43587 113683 +05 1168 0 1180R 5 F8 +44.0 0.140 -- 2313 45067 133229 -00 1287 1190S 5 M1 -53.0 ----- 239 ------+17 1320 120G104-49
1200S 5 K6 -44.8 0.517 241 - 47752 78637 +24 1357 120G109-20 1210S 4 F5 +25 0.237 242 2484 48737 96074 +13 1396 N 1220S 5 GO -23.7 0.158 245 2483 48682 41330 +43 1595 0 1230S 5 MO p -48.4 0.706 247 -- 48948 13971 +60 1003 1240S 5 K6 +26.8 1.048 249 - 49601 ------+47 1355 120G107-27
1250S 5 K6 -10.3 ----- 250A ---- 50281 133805 -05 1844 Y 1260S 5 M4 +36.0 0.723 251 ------112G087-12 1270S 5 G4 +25.9 0.361 9220B ------S 1280S 5 GO -11.3 0.161 252 2569 50692 78866 +25 1496 1290S 5 KO e +12.6 259 ---- 52698 172768 -25 3913
1300S 5 M5 e +39.0 ----- 268 ------112G087-26 S 1310S 5 GO p +85.0 ------2721 55575 41644 +47 1419 1320S 5 K8 + 1.5 0.542 9233 ---- 58830 60106 +32 1559 G090-01 C 1330S 5 M4 +26.0 0.850 273 ------+05 1668 112G089-19 A 1340S 4 F7 +61.1 ----- 279 2906 60532 174009 -21 2007
1350S 4 F6 +46 ------2927 61064 134899 -03 1979 0 1360S 4-5 F5 - 3.0 0.189 280A 2943 61421 115756 +05 1739 S 1370S 5 MO + 9.8 0.617 281 ------+02 1729 120G112-35 1380S 5 K2 e -21.1 ----- 282A ---- 61606 134954 -03 2001 120G112-37 Y 1390S 5 K5 -11.4 ----- 282B ------03 2002 G112-38 Y
1400S 4 G1 -36.0 0.138 --- 3176 67228 79959 +22 1862 1410S 5 G8 +29.7 ----- 302 3259 69830 154093 -12 2449 1420S 5 F6 +32.5 0.154 303 3262 69897 80104 +27 1589 1430S 5 M1 +15.0 -- 310 ------+67 0552 G234-38 Y 1440S 5 GO -12.0 0.395 311 3391 72905 14609 +65 0643
1450S 5 F7 + 5.0 0.270 3499 75332 61074 +33 1765 1460S 5 MO -21.0 1.720 322 ------+66 0582 1470S 5 G8 +26.6 ----- 324A 3522 75732 80478 +28 1660 C 1480S 5 K5 +47.5 1.510 325A ---- 75632 6683 +71 0482 Y 1490S 5 G3 +28.0 0.260 327 3538 76151 136389 -04 2490
1500S 5 F6 p 121.0 ----- 3578 76932 154804 -15 2656 1510S 5 F9 e +27.0 0.240 334.2 3625 78366 61288 +34 1949 1520S 5 MO e +10.5 2.113 338A ---- 79210 27178 +53 1320 136G195-17 Y 1530S 5 MOe + 9.4 1.955 338B ---- 79211 27179 +53 1321 136G195-18 Y 1540S 5 K5 e - 2.1 ----- 342 ---- 80768 6853 +76 0351 ------20
HAO # RA DEC PMa PMS PAR V B-V U-B R-I I
1550S 09 26 36.6 -02 32 58 +0.0084 -0.018 0.071 4.60 0.46 0.00 0.22 3.96 1560S 09 26 37.0 -02 31 54 +0.0099 -0.018 0.071 7.19 0.87 0.57 1570S 09 27 18.6 +05 52 24 -0.0345 +0.089 0.088 7.21 1.00 0.87 1580S 09 30 54.2 -20 53 37 -0.0020 +0.010 0.051 5.01 1.02 0.87 -- 1590S 09 32 40.0 +36 02 15 -0.0582 -0.248 0.109 5.41 0.77 0.44 0.37 4.42
1600S 09 34 25.0 +22 55 42 -0.0100 -0.190 0.046 9.50 1.29 1.28 ---- 1610S 09 39 58.9 -23 41 25 -0.0291 +0.255 0.079 4.94 0.53 0.00 0.28 4.13 1620S 09 40 16.7 +42 55 56 +0.0040 -0.828 0.069 8.12 1.15 1.15 0.42 1630S 09 45 22.4 +46 15 18 +0.0216 -0.095 0.066 5.09 0.62 0.10 0.34 4.23 1640S 09 49 36.9 +03 27 25 -0.0292 +0.019 0.044 8.89 1.23 1.23 0.47 -
1650S 09 52 29.0 +63 02 00 -0.0500 -0.600 0.083 8.99 1.44 1.19 0.73 - 1660S 09 58 08.0 +32 10 14 -0.0414 -0.433 0.054 5.36 0.66 0.27 -- 1670S 10 08 19.1 +49 42 29 -0.1404 -0.509 0.222 6.59 1.35 1.28 0.80 4.56 1680S 10 09 46.0 -03 29 42 -0.0100 -0.210 0.105 9.30 1.47 1.22 0.92 - 1690S 10 11 44.8 +21 25 03 -0.0101 -0.087 6.02 0.56 ------
1700S 10 13 46.3 +23 45 08 -0.0149 +0.031 0.034 5.97 0.67 ---- 1710S 10 16 54.0 +20 07 18 -0.0346 -0.050 0.206 9.43 1.54 1.08 1.12 - 1720S 10 17 01.0 +19 43 31 -0.0165 -0.220 0.051 4.79 0.45 0.01 0.23 4.12 1730S 10 19 12.6 +41 29 03 -0.0111 -0.141 0.042 5.76 0.54 0.08 -- 1750S 10 26 23.0 +01 06 24 -0.0410 -0.760 0.130 9.63 1.52 1.19 0.95 -
1760S 10 27 14.0 +56 15 24 -0.0200 -0.060 0.093 8.69 1.36 1.26 0.55 - 1770S 10 27 26.4 +56 14 16 -0.0214 -0.035 0.081 4.84 0.52 -.01 0.28 4.08 1780S 10 28 27.0 +45 47 30 -0.0550 -0.580 0.067 8.84 1.34 1.27 0.59 - 1790S 10 51 02.6 -19 52 09 +0.0053 -0.244 0.052 5.24 0.47 0.06 - 1800S 10 56 40.3 +40 41 52 -0.0281 +0.051 0.074 5.05 0.61 0.13 0.31
1810S 10 57 25.0 +23 06 18 -0.0290 -0.280 0.151 10.04 1.54 1.22 1.02 - 1820S 10 59 57.0 +22 14 12 +0.0110 -0.040 0.088 9.52 1.47 ------1830S 11 00 36.6 +36 18 20 -0.0468 -4.743 0.396 7.49 1.51 1.13 0.91 4.78 1840S 11 03 00.0 +43 47 00 -0.4094 +0.936 0.192 8.76 1.54 1.18 0.82 - 1850S 11 08 20.5 +30 43 13 +0.0447 -0.208 0.081 8.38 1.34 1.27 0.59 -
1860S 11 09 49.3 +36 05 17 -0.0225 -0.175 0.042 6.41 0.61 0.10 - 1870S 11 10 39.4 +04 45 18 -0.0205 -0.034 0.054 8.73 1.17 1.09 0.46 1880S 11 11 57.3 +73 44 47 -0.0955 +0.105 0.079 7.72 1.04 -.92 0.40 - 1890S 11 13 57.0 -14 25 00 -0.0140 -0.100 0.040 10.00 1.30 ------1900S 11 17 29.0 +66 07 00 -0.4854 +0.149 0.119 9.32 1.42 1.08 0.76
1910S 11 24 13.4 +03 17 09 -0.0483 +0.177 0.057 6.50 0.79 0.49 0.36 1920S 11 24 14.4 +03 16 43 -0.0484 +0.169 0.057 7.60 1.00 0.92 ---- 1930S 11 29 09.5 +14 38 50 -0.0214 -0.172 0.035 6.20 0.57 0.07 ------1940S 11 31 48.4 +03 20 17 -0.0123 -0.107 0.044 5.77 0.46 0.01 ---- - 1950S 11 38 25.3 +34 29 03 -0.0010 -0.388 0.110 5.33 0.72 0.25 0.36 4.37 21
HAO # SPEC RV HK W# BS # HD # SAO # BD # FIND CHART BIN I C
1550S 5 F6 + 9.8 0.206 348A 3759 81997 136895 -02 2901 C 1560S KO +22.5 ----- 348B ------...----. . --02 2902 1570S 5 K3 e +26.7 0.797 349 - 82106 117737 +06 2182 C 1580S 4 KO +13.3 ----- 9302 3808 82734 177642 -20 2936 1590S 4 G8 e +13.4 0.315 356A 3815 82885 61586 +36 1979 Y
1600S 5 K8 -32.5 ----- 9304 ...... ------.---- +23 2121 1610S 5 GO +33.8 ----- 364 3862 84117 177866 -23 8646 1620S 5 K5 -13.4 -- 365 - 84035 42997 +43 1953 120G116-42 1630S 5 G2 + 5.2 0.144 368 3881 84737 43046 +46 1551 1640S 5 MOp +18.1 ----- 371 - 85488 117958 +03 2279 102G048-45
1650S 5 M1 +10.6 ----- 373 -.---- +63 0869 144G235-49 1660S 5 G2 +56.0 0.156 376 3951 86728 61808 +32 1964 0 1670S 5 K7 e -26.0 1.617 380 - 88230 43223 +50 1725 136G196-09 Y 1680S 5 M2 +12.2 ----- 382 -03 2870 112G053-29 U 1690S5 F9 +17.0 0.235 ---- 4012 88737 81250 +21 2165 ------
1700S 4 G2 p -33.0 --- 4030 89010 81260 +24 2207 S 1710S 5 M4 e + 9.9 ----- 388 ...... -- ..------+20 2465 112G054-23 Y 1720S 4 F6 + 6.9 0.178 9324 4054 89449 99065 +20 2466 1730S 5 F6 - 6.5 0.135 9326 4067 89744 43309 +41 2076 1750S 5 M2 +11.6 1.035 393 ------. ------+01 2447 112G055-24
1760S 5 K7 e + 3.0 1.687 394 ---. ------+56 1458 Y 1770S 5 F8 + 9.2 0.199 395 4112 90839 27670 +56 1459 A 1780S 5 K7 +22.8 1.677 397 ------.. ------+46 1635 120G146-39 1790S 5 F6 - 4.8 ----- 9338 4251 94388 156301 -19 3125 0 1800S SGO +12.6 0.165 407 4277 95128 43557 +41 2147
1810S 5 M3 +29.0 ----- 408 112G058-32 1820S 5 M2 e -20.0 ----- 410 ---- 95650 ------+22 2302 1830S5 M2 e -86.5 0.396 411 ---- 95735 62377 +36 2147 120G119-52 A 1840S 5 M2 e +64.9 -- 412A ------+44 2051 129G176-11 0 1850S 5 K9 e -14.0 -- 414A ---- 97101 62440 +31 2240 120G119-60 Y
1860S 5 GO - 2.6 0.320 417 4345 97334 62451 +36 2162 Y 1870S 5 K5 +19.0 -- 418 - 97503 118726 +05 2463 102G010-07 1880S 5 K5 + 8.1 0.585 420A - 97584 7320 +74 0456 0 1890S 5 MO ...... 9355 ...... -13 3333 1900S 5 M1 +46.9 -- 424 ------...... - +66 0717 ------
1910S 4 KO - 2.9 ----- 429A 4414 99491 118864 +03 2502 0 1920S 5 K2 + 1.7 -- 429B 99492 118865 +03 2503 102GO10-23 0 1930S 5 GO - 4.0 0.165 - 4437 100180 99647 +15 2345 0 1940S5 F5 + 3.0 0.195 9367 4455 100563 118929 +03 2521 1950S 5 G8 e - 5.4 0.310 434 4496 101501 62655 +35 2270 ------Y 22
HAO # RA DEC PMa PMS PAR V B-V U-B R-I I
1960S 11 43 08.0 +72 22 18 +0.0040 +0.060 0.054 9.02 1.17 1.12 0.46 1970S 11 45 09.0 +01 06 00 +0.0420 -1.250 0.301 11.10 1.76 1.40 1.30 1980S 11 48 05.4 +02 02 48 +0.0494 -0.275 0.100 3.61 0.55 0.11 0.28 2.84 1990S 11 50 06.2 +38 04 39 +0.3387 -5.806 0.110 6.45 0.75 0.17 0.45 5.35 2000S 11 58 10.4 -10 09 40 +0.0082 -0.482 0.080 5.55 0.77 0.44 0.36 -
2010S 12 12 36.0 -10 01 14 +0.0020 -1.023 0.034 6.11 0.46 -.13 0.16 - 2020S 12 16 59.4 +28 26 10 -0.0150 -0.133 0.025 6.33 0.50 - 2030S 12 19 25.0 +42 25 06 +0.0190 -0.530 0.070 9.48 1.35 1.21 0.60 - 2040S 12 31 22.3 +41 37 44 -0.0631 +0.288 0.109 4.26 0.59 0.05 0.31 3.42 2050S 12 38 35.5 +15 39 22 +0.0073 -0.419 0.087 8.00 1.12 1.00 0.44 -
2060S 12 41 58.8 +52 02 06 -0.0431 -0.193 0.063 7.04 0.94 0.71 - 2070S 12 48 09.7 -00 29 26 -0.0029 -0.395 0.091 8.49 1.41 1.27 0.66 - 2080S 12 55 19.0 +35 29 48 -0.0220 -0.190 0.057 10.60 1.42 1.13 0.80 2090S 12 57 45.2 -02 26 08 -0.0535 +0.006 0.054 9.81 1.16 1.15 0.50 - 2100S 13 03 49.0 +20 59 42 -0.0040 +0.060 0.059 9.43 1.29 1.22 0.60
2110S 13 05 15.0 +34 40 06 -0.0103 -0.005 0.051 9.34 1.18 1.10 - 2120S 13 07 33.3 +17 47 36 -0.0302 +0.131 0.054 4.32 0.45 -.06 2130S 13 09 23.6 -15 55 46 +0.0065 -0.292 0.040 5.04 0.46 0.02 -- 2140S 13 09 32.4 +28 07 52 -0.0605 +0.879 0.120 4.26 0.57 0.07 0.30 3.47 2150S 13 13 16.2 -19 40 40 +0.0215 -0.121 0.046 5.22 1.03 0.87 --
2160S 13 14 17.5 +09 41 06 -0.0227 +0.187 0.077 5.22 0.59 0.10 0.20 2170S 13 14 21.8 +17 17 03 +0.0440 -0.270 0.087 6.52 0.94 0.61 -- 2180S 13 15 47.1 -18 02 01 -0.0754 -1.072 0.119 4.74 0.71 0.26 0.36 3.80 2190S 13 17 14.0 +35 23 00 +0.0331 -0.790 0.099 9.52 1.47 1.18 0.82 - 2200S 13 25 59.0 +14 02 43 -0.0164 -0.581 0.041 4.98 0.71 0.26 0.39 3.98
2210S 13 27 27.0 +10 39 00 +0.0670 -0.99 0.131 9.04 1.51 1.24 0.82 - 2220S 13 30 54.0 +43 31 36 +0.0027 -0.035 0.040 9.40 1.08 0.91 - 2230S 13 32 06.6 -08 05 07 -0.0186 -0.098 0.061 9.34 1.18 1.05 0.54 - 2240S 13 43 11.8 +15 09 43 +0.1228 -1.454 0.205 8.46 1.45 1.08 0.85 5.92 2250S 13 44 53.1 +17 42 19 -0.0338 +0.034 0.057 4.50 0.48 0.04 0.24 3.85
2260S 13 47 05.1 -21 51 23 -0.1261 -0.502 0.080 8.16 1.29 1.30 - 2270S 13 47 09.0 -17 53 09 -0.0071 -0.041 0.044 4.97 1.06 0.92 0.50 - 2280S 13 50 01.0 +50 11 54 +0.045 -0.16 0.076 8.90 1.33 1.20 0.58 - 2290S 13 52 18.2 +18 38 51 -0.0045 -0.363 0.102 2.68 0.58 0.20 0.29 1.95 2300S 14 01 04.8 +11 01 50 +0.0055 -0.311 0.061 6.30 0.74 0.29 0.40 ---
2310S 14 11 40.8 +13 11 35 -0.0176 -0.055 0.022 5.54 0.54 0.09 - 2320S 14 13 23.3 -05 45 46 -0.0006 -0.432 0.043 4.08 0.52 0.04 0.27 3.32 2330S 14 16 20.0 -06 22 06 +0.0000 -0.400 0.046 9.12 1.30 1.20 ---- - 2340S 14 19 48.0 +29 51 42 -0.0509 -0.314 0.073 8.54 1.26 1.24 0.52 - 2350S 14 20 41.7 +01 28 30 +0.0148 -0.481 0.061 6.27 0.63 0.09 0.32 5.39 23
HAO # SPEC RV HK W # BS # HD # SAO # BD # FIND CHART BIN
1960S 5 K8 -23.6 1.082 441 ...... +72 0545 1970S 5 M5 -13.0 447 102G010-50 1980S 5 F8 + 4.7 449 4540 102870 119076 +02 2489 Y 1990S 5 G8 p -98.3 0.180 451A 4550 103095 62738 +38 2285 G122-51 S 2000S 5 G7 + 0.4 0.151 454 4587 104304 157041 -09 3413
2010S 5 F5 + 8.0 0.208 4657 106516 157168 -09 3468 Y 2020S 5 F8 - 8.0 0.138 4688 107213 82244 +28 2106 2030S 5 MO e +14.7 1.471 462 - 107596 ------+42 2296 120G123-26 2040S 5 GO + 6.9 0.177 475 4785 109358 44230 +42 2321 S 2050S 5 K8 +23.5 -- 481 - 110315 100205 +16 2404 112G059-33
2060S 5 KO e + 8.6 0.314 483 - 110833 28499 +52 1650 136G199-36 2070S 5 MO e + 2.8 1.586 488 - 111631 138992 +00 2989 102G014-06 2080S 5 MO e -10.0 7.214 490A -...... +36 2322 120G123-75 O 2090S 5 MO -12.3 493 - 112943 139091 -01 2754 102G014-19 2100S 5 MO - 4.5 499A - ...... -- +21 2486 ------0
2110S 5 K8 - 7.8 1.038 9427 ...... +35 2406 2120S 5 F5 -17.7 0.240 501A 4968 114378 100443 +18 2697 S 2130S 3-4 F5 -14.0 4981 114642 157788 -15 3613 Y 2140S 5 GO +6.1 0.200 502 4983 114710 82706 +28 2193 S 2150S 4 K1 +34.1 9435 5001 115202 157823 -19 3653
2160S 5 GO -25.9 0.310 504 5011 115383 119847 +10 2531 Y 2170S 5 K2 + 5.5 0.550 505A - 115404 100491 +17 2611 112G063-18 0 2180S 5 G6 - 8.5 0.160 506 5019 115617 157844 -17 3813 Y 2190S 5 MO - 2.9 1.417 507A ...... +35 2436 124G 164-64 0 2200S 4-5 G5 + 4.2 0.143 9446 5072 117176 100582 +14 2621 Y
2210S 5 M1 +16.2 1.083 514 ...... +11 2576 112G063-34 2220S 5 K8 - 3.7 1.037 9449 ------...- +44 2279 2230S 5 K5 e -20.1 517 - 118100 139419 -07 3646 2240S 5 M4 e +15.2 0.948 526 - 119850 100695 +15 2620 112G063-53 2250S 5 F7 -15.6 0.185 527A 5185 120136 100706 +18 2782 Y
2260S 5 K6 -35.3 529 - 120467 181997 -21 3781 2270S 3 K1 -39.7 9460 5196 120452 158186 -17 3937 2280S 5 MO p -41.4 532 ...... +50 2030 129G177-62 2290S 4 GO - 0.1 534 5235 121370 100766 +19 2725 S 2300S 5 G8 -17.0 0.181 538 5273 122742 100832 +11 2625 A
2310S 4 F6 -39.0 0.135 5323 124570 100925 +13 2764 S 2320S 3 F6 +11.5 0.208 9473 5338 124850 139824 -05 3843 2330S 5 MO p +13.8 9477 - 125354 ------05 3853 G124-22 2340S 5 K8 -38.2 1.406 546 ------+30 2512 124G166-22 2350S 5 G1 -17.5 0.170 547 5384 126053 120424 +01 2920 112G065-47 24
HAO # RA DEC PMa PM8 PAR V B-V U-B R-I I
2360S 14 23 29.6 +52 04 52 -0.0262 -0.400 0.068 4.05 0.50 0.01 0.25 3.39 2370S 14 25 37.4 -02 00 17 -0.0094 -0.005 0.045 4.81 0.70 0.21 0.37 3.87 2380S 14 28 12.2 -08 25 18 -0.0851 -0.226 0.052 9.45 1.40 1.20 0.66 - 2390S 14 28 42.2 +35 40 19 -0.0397 +0.190 0.054 8.70 1.13 ------2400S 14 31 50.9 +53 07 27 -0.0233 +0.240 0.071 7.23 0.99 0.84 -
2410S 14 44 03.0 +16 43 06 -0.0088 -0.928 0.072 9.26 1.28 1.16 0.53 2420S 14 48 49.9 -24 05 35 -0.0676 -0.422 0.069 7.83 1.02 0.88 -- 2430S 14 49 04.8 +19 18 27 +0.0096 -0.103 0.148 4.74 0.76 0.28 0.43 3.48 2440S 14 49 05.0 +19 18 24 +0.0095 -0.107 0.148 6.97 1.17 ------2450S 14 54 31.0 -21 11 18 +0.0696 -1.668 0.180 8.02 1.54 1.20 0.89 5.47
2460S 14 54 32.4 -21 11 28 +0.0745 -1.740 0.180 5.74 1.11 1.06 0.56 4.18 2470S 14 54 43.4 +49 49 56 +0.0108 -0.226 0.027 5.63 0.50 0.00 -- 2480S 14 58 00.6 -10 55 52 +0.0004 -0.469 0.051 9.49 1.38 1.29 -- 2490S 14 59 09.0 +45 37 06 +0.0250 +0.340 0.069 9.13 1.43 1.18 0.72 2500S 15 05 06.2 +25 03 46 +0.0136 -0.171 0.062 4.93 0.43 -.02 0.21 4.32
2510S 15 14 03.2 +67 32 11 +0.0368 -0.393 0.047 5.13 0.53 0.08 -- 2520S 15 16 45.4 +01 57 12 +0.0247 -0.518 0.037 5.06 0.54 0.06 0.27 4.38 2530S 15 19 27.0 -04 35 54 -0.0200 +0.010 0.059 9.47 1.30 1.22 0.56 - 2540S 15 21 29.0 -10 08 38 -0.0048 -0.158 0.035 4.94 0.44 0.02 -- 2550S 15 34 09.8 +39 59 42 -0.0394 +0.056 0.053 7.62 0.95 0.76 0.29 -
2560S 15 40 22.5 -10 46 18 -0.0776 -0.317 7.24 0.49 -.91 ---- 6.31 2570S 15 44 00.8 +07 30 31 -0.0151 -0.068 0.094 4.43 0.60 0.11 0.32 3.60 2580S 15 49 20.8 +35 48 41 -0.0010 -0.351 0.034 4.82 1.00 0.87 0.49 3.57 2590S 15 50 56.7 +42 35 26 +0.0396 +0.628 0.056 4.62 0.56 0.00 0.32 3.82 2600S 15 54 08.5 +15 49 25 +0.0212 -1.285 0.081 3.85 0.48 -.03 0.24 3.13
2610S 15 59 07.8 +33 27 12 -0.0159 -0.768 0.042 5.41 0.60 0.08 0.32 - 2620S 16 02 43.9 -20 18 37 +0.0228 -0.341 0.058 7.10 1.04 1.07 - 2630S 16 03 58.3 +80 45 51 -0.0111 +0.016 0.046 7.60 1.06 ------2640S 16 08 46.8 +43 57 02 +0.0114 -0.304 0.063 6.67 0.90 0.65 - 2650S 16 12 54.0 -08 14 19 +0.0154 -0.505 0.061 5.50 0.65 0.17 0.33 -
2660S 16 16 36.9 +67 21 32 -0.0899 +0.086 0.089 8.62 1.41 1.26 0.68 6.40 2670S 16 19 12.0 +41 04 36 +0.0000 +0.080 0.064 8.98 1.30 1.17 0.56 - 2680S 16 25 31.9 +07 25 09 -0.0178 -0.270 0.058 8.88 1.22 1.20 0.50 2690S 16 33 44.0 -02 13 12 +0.0301 -0.317 0.090 5.75 0.82 0.48 0.39 4.74 2700S 16 43 14.6 +33 35 39 -0.0037 +0.375 0.104 8.11 1.37 1.29 0.57 -
2710S 16 50 27.4 +00 04 32 -0.0481 -1.505 0.067 6.64 0.76 0.32 0.24 - 2720S 16 52 48.5 -08 14 42 -0.0537 -0.875 0.156 9.01 1.62 1.09 1.08 5.98 2730S 16 56 07.0 +25 49 36 -0.008 -0.54 0.085 9.72 1.50 1.20 0.86 - 2740S 17 02 27.0 -04 58 58 -0.0622 -1.127 0.086 7.74 1.16 1.05 0.49 6.00 2750S 17 02 44.0 +00 46 28 -0.0005 -0.339 0.049 6.01 0.58 0.06 ---- 25
HAO # SPEC RV HK W# BS # HD # SAO # BD # FIND CHART BIN
2360S 5 F6 -10.9 0.246 549A 5404 126660 29137 +52 1804 Y 2370S 3 G2 - 9.5 -- 9481A 5409 126868 139951 -01 2957 0 2380S 5 K7 -26.8 553 - 127339 139977 -07 3856 120G124-47 U 2390S 5 K5 -12.0 0.665 554 - 127506 64191 +36 2500 129G178-31 2400S 5 K3 +14.1 0.305 556 - 128165 29196 +53 1719 136G200-49
2410S 5 K5 +47.8 - 562 .. . ---. +17. 2785 120G136-13 2420S 5 K5 -65.0 0.400 565 130992 182935 -23 11940 2430S 5 G8 e + 3.9 0.450 566A 5544 131156 101250 +19 2870 0 2440S 5 K5 e + 5.4 1.400 566B - 131156 101250 +19 2870 0 2450S 5 M2 +25.9 570B - 131976 183039 -20 4123 ------0
2460S 5 K5 e +19.5 -- 570A 5568 131977 183040 -20 4125 0 2470S 5 F7 -15.0 5581 132254 45288 +50 2126 2480S 5 MO +14.0 9507 - 132683 158967 -10 4011 G151-18 2490S 5 MO -14.8 1.616 572 ------..-- ...-- - +45 2247 129G179-06 2500S 5 F5 - 7.3 0.207 578 5634 134083 83671 +25 2873 0
2510S 5 F8 -46.8 0.135 9517 5691 136064 16660 +67 0876 2520S 3-4 F8 +54.0 0.140 5694 136202 120946 +02 2944 Y 2530S 5 K6 -15.0 583 ...... ------04 3873 102G015-19 2540S 4 F5 p -10.0 5723 137052 159234 -09 4138 S 2550S 5 K5 -71.5 0.187 591 - 139323 64799 +40 2903 129G179-37 Y
2560S 5 K5 p - 140283 159459 -10 4149 2570S 5 GO -66.4 0.160 598 5868 141004 121186 +07 3023 S 2580S 4K1 -24.0 5901 142091 64948 +36 2652 Y 2590S 5 F9 -55.2 0.142 602 5914 142373 45772 +42 2648 2600S 5 F6 + 6.7 0.155 603 5933 142860 101826 +16 2849 O
2610S 5 G2 +18.4 0.150 9537 5968 143761 65024 +33 2663 0 2620S 5 K2 +34.0 610 - 144253 184105 -20 4399 2630S KO -36.0 0.111 9545 - 145742 2652 +81 0541 2640S 5K1 - 5.5 0.151 614 145675 45933 +44 2549 129G180-35 2650S 5G1 +10.6 0.174 616 6060 146233 141066 -07 4242 0
2660S 5 MO e -13.8 1.761 617A - 147379 17026 +67 0935 140G225-57 0 2670S 5 MO p + 4.9 0.897 619 ....-- .... +41 2695 2680S 5 K8 -31.8 0.749 626 - 148467 121619 +07 3180 102G017-18 2690S 5 KO e -15.4 0.360 631 6171 149661 ---- -02 4211 2700S 5 K7 -30.5 1.379 638 - 151288 65525 +33 2777 G181-06
2710S 5 G6 +41.2 0.400 641 152391 121921 +00 3593 G019-04 2720S 5 M3 e +19.0 -- 644A 152751 141439 -08 4352 S 2730S 5 M2 + 6.4 1.912 649 ------...- +25 3173 124G 169-38 2740S 5 K5 +28.5 653 - 154363 141508 -04 4225 102G019-13 C 2750S 5 F8 -17.5 0.275 9583 6349 154417 122056 +00 3629 ------26
HAO # RA DEC PMa PM8 PAR V B-V U-B R-I I
2760S 17 09 07.8 +54 33 24 +0.0101 -0.116 0.049 8.83 1.16 1.07 0.45 - 2770S 17 09 10.0 +54 33 06 +0.0110 -0.130 0.049 9.34 1.26 1.19 0.50 2780S 17 13 08.7 -26 28 33 -0.0359 -1.124 0.178 6.34 1.16 1.07 0.65 2790S 17 18 00.3 -21 03 40 +0.0165 -0.209 0.060 4.39 0.39 -.05 0.22 3.79 2800S 17 18 47.2 +32 31 51 +0.0100 -1.043 0.073 5.39 0.62 0.07 0.35
2810S 17 23 15.9 +02 10 14 -0.0391 -1.193 0.132 7.53 1.36 1.26 0.60 1.26 2820S 17 23 18.8 -24 07 52 +0.0000 -0.116 0.045 4.17 0.28 0.12 0.12 3.75 2830S 17 23 22.0 -01 36 35 +0.0042 +0.048 - 6.44 0.46 -.02 -- 2840S 17 25 55.0 +05 35 24 +0.0010 -0.270 0.104 9.32 1.47 1.24 2850S 17 27 49.2 -01 01 22 -0.0080 -0.170 0.052 5.31 0.72 0.31 0.36 -
2860S 17 31 12.3 +19 17 29 -0.0022 -0.093 0.032 5.64 0.48 -.02 - 2870S 17 35 39.0 +18 36 24 +0.0650 +0.990 0.126 9.62 1.53 1.08 0.88 2880S 17 36 47.9 +03 34 59 -0.0120 -0.100 0.081 6.52 0.96 0.78 0.50 2890S 17 37 01.7 +71 54 26 +0.0162 -0.051 0.047 8.62 1.10 1.04 0.43 - 2900S 17 41 18.3 +24 20 53 -0.0085 +0.071 0.006 5.71 0.65 0.27 0.33 -
2910S 17 42 50.9 +72 10 55 +0.0041 -0.278 0.054 5.79 0.53 0.02 - .-- 2920S 17 44 30.0 +27 44 55 -0.0233 -0.747 0.128 3.42 0.75 0.39 0.38 2.51 2930S 17 51 41.0 +76 58 15 +0.0105 +0.246 0.032 5.04 0.49 0.08 -- 2940S 17 55 23.0 +04 33 18 -0.0500 +10.31 0.548 9.54 1.74 1.29 1.23 - 2950S 18 02 28.3 -03 01 53 +0.0368 -0.333 0.138 9.38 1.52 1.21 0.88 -
2960S 18 02 55.6 +02 30 35 +0.0172 -1.094 0.195 4.03 0.86 0.54 0.46 2.92 2970S 18 03 47.4 +79 59 48 +0.0164 +0.127 0.025 6.04 0.51 -.01 -- 2980S 18 03 53.5 +79 59 60 +0.0155 +0.120 0.025 5.68 0.50 -.01 -- 2990S 18 05 10.0 +15 56 54 +0.0060 +0.000 0.055 8.17 1.32 -- - 3000S 18 07 58.0 +38 27 12 -0.0264 -0.471 0.093 6.40 0.87 0.59 0.49 5.14
3010S 18 13 36.4 +64 22 48 +0.0526 +0.032 0.047 5.03 0.38 -.04 -- 3020S 18 27 15.9 -01 51 00 +0.0116 -0.207 0.054 8.05 1.10 1.06 - 3030S 18 28 22.9 -18 56 32 -0.0099 -0.195 0.078 6.82 0.84 0.65 0.30 - 3040S 18 30 42.0 -11 40 18 -0.0210 -0.270 0.054 10.01 1.28 1.19 0.53 --. 3050S 18 34 04.6 +09 04 54 -0.0006 -0.129 0.033 5.39 0.37 -.02 -
3060S 18 34 13.1 +06 37 51 -0.0019 -0.140 0.032 5.45 0.37 -.04 3070S 18 35 54.5 -21 05 42 -0.0057 -0.152 0.067 5.86 0.68 0.14 - 3080S 18 42 12.9 +59 32 59 -0.1794 +1.818 0.284 8.90 1.54 1.11 1.07 5.39 3090S 18 42 14.0 +59 33 00 -0.1790 +1.815 0.284 9.69 1.59 1.14 1.14 - 3100S 18 43 30.5 +20 29 50 -0.0008 -0.334 0.049 4.19 0.46 0.01 0.26 3.54
3110S 18 44 49.8 -03 41 29 -0.0082 -0.247 0.075 8.82 1.28 1.22 0.54 - 3120S 18 46 07.5 +10 41 40 +0.0096 -0.439 0.059 7.99 1.06 0.98 0.38 - 3130S 18 46 40.0 +17 23 15 -0.0292 -0.401 0.061 9.20 1.29 1.22 0.60 3140S 18 49 38.0 +16 31 48 -0.0180 -0.430 0.079 10.10 1.57 ------3150S 18 50 27.7 +52 54 35 -0.0054 +0.272 0.037 5.51 0.84 0.51 0.42 --- 27
HAO # SPEC RV HK W# BS # HD # SAO # BD # FIND CHART BIN
2760S 5 K8 + 5.9 1.290 659A ---- 155674 30274 +54 1861 Y 2770S 5 K8 - 0.4 3.061 659B ------+54 1862 Y 2780S 5 K5 e - 1.3 0.835 664 ---- 156026 185213 -26 12036 A 2790S 5 F2 -9.1 -- 670A 6445 156897 185296 -20 4731 Y 2800S 5G1 -78.4 0.156 672 6458 157214 65963 +32 2896 0
2810S 5 K7 -28.3 1.464 673' ---- 157881 122374 +02 3312 102G019-24 2820S 5 A9 -37.2 -- 9591 6486 157792 185401 -24 13337 2830S 5 F3 -24.0 0.196 ----- 6489 157856 141661 -01 3329 2840S 5 M1 e -11.2 1.436 9592 ------+05 3409 G139-43 0 2850S 4-5 G8 -77.0 0.165 678AB 6516 158614 141702 -00 3300 ------r S
2860S 5 F6 -59.0 0.145 6541 159332 102912 +19 3354 2870S 5 Ml - 9.8 1.046 686 ...... - - .....-- - +68 0946 124G170-55 A 2880S 5 K3 +19.1 0.305 688 160346 122610 +03 3465 2890S 5 K4 -23.6 .---- 689 - 160964 8855 +71 0850 2900S 3 G2 -26.0 0.140 --- 6608 161239 85360 +24 3237
2910S 5 GO -10.0 0.159 9602B 6637 162004 8891 +72 805 0 2920S 4 G5e -15.6 ----- 695A 6623 161797 85397 +27 2888 0 2930S 4 F6 p +23.0 6701 163989 8939 +76 0667 2940S 5 M5 -109 0.772 699 ...... +04 3561 G140-24 A 2950S 5 M2 +34.0 ----- 701 - 165222 142072 -03 4233 102G020-22
2960S 5 KOe - 7.2 0.385 702A 6752 165341 123107 +02 3482 G205-30 S 2970S F7 p +4.0 6809 166865 8994 +79 0570 S 2980S F7 p +10.0 6810 166866 8996 +79 0571 S 2990S K2 p -38.0 0.135 705 ...... ----..... - +15 3367 3000S 5 K2 -18.7 0.205 706 6806 166620 66700 +38 3095 G205-05
3010S 5 F5 -35.3 0.210 9619 6850 168151 17828 +64 1252 3020S 5 K5 -53.3 .. 715 - 170493 142350 -01 3500 102G021-17 3030S 5 K3 -46.5 -- 716 - 170657 161557 -18 4986 3040S 5 MO -83.7 .. 717 ------11 4672 122G155-23 3050S 3 F5 p -22.0 6985 171802 123690 +09 3783 ------
3060S 5 F3 -21.0 6987 171834 123693 +06 3855 S 3070S 5 G4 +35.6 722 6998 172051 187086 -21 5081 3080S 5 M4 - 0.2 0.439 725A 173739 31129 +59 1915 G227-46 0 3090S 5 M5 +10.0 0.494 725B 173740 --..-- G227-47 0 3100S 5 F6 +23.7 0.190 9635 7061 173667 86406 +20 3926 ------0
3110S 5 MOp +17.7 726 - 173818 142621 -03 4380 102G021-24 3120S 5 K4 -17.9 0.793 727 - 174080 104119 +10 3665 120G141-37 0 3130S 5 M1 -16.7 1.062 728 - 229590 104126 +17 3729 132G184-29 3140S 5 M2 e -11.0 1.432 731 - 229793------132G184-35 3150S 4 G9 + 2.0 -- 732.1 7123 175225 31217 +52 2294 28
HAO # RA DEC PMa PM5 PAR V B-V U-B R-I I
3160S 18 53 03.0 +08 20 18 +0.0070 -0.080 0.092 10.07 1.75 3170S 18 55 09.0 +32 50 10 +0.0133 -0.157 0.054 5.22 0.59 0.02 0.34 - 3180S 18 55 33.7 +05 51 24 -0.0139 -1.218 0.085 9.23 1.45 1.30 0.76 3190S 18 55 57.0 +06 10 22 -0.0004 -0.103 ---- 6.21 0.46 0.01 --- 3200S 18 56 47.5 +13 33 16 +0.0008 -0.122 0.039 5.23 0.53 0.07 0.30 4.50
3210S 19 05 06.0 +20 48 06 -0.0340 -0.320 0.119 10.76 1.56 ---- 0.96 - 3220S 19 11 01.1 +76 28 42 +0.0127 -0.121 0.046 5.13 0.31 0.00 0.17 4.66 3230S 19 14 29.0 +05 05 48 -0.0390 -1.340 0.172 9.12 1.49 1.15 1.00 - 3240S 19 20 25.5 +09 48 52 +0.0008 +0.097 --- 6.35 0.44 -.03 - - 3250S 19 21 40.7 +33 07 18 +0.0066 +0.168 0.057 6.37 0.81 0.46 --
3260S 19 22 35.1 +11 50 09 +0.0492 +0.640 0.060 5.16 0.77 0.42 - 3270S 19 32 09.2 +04 28 04 +0.0356 +0.308 0.078 9.36 1.39 1.23 0.61 - 3280S 19 32 27.6 +69 34 34 +0.1098 -1.744 0.176 4.68 0.79 0.38 0.41 3.63 3290S 19 35 06.0 +50 06 16 -0.0025 +0.256 0.056 4.48 0.38 -.03 0.21 3.91 3300S 19 35 08.1 -04 45 38 +0.0069 -0.050 0.027 5.46 0.43 0.03 --
3310S 19 40 29.1 +50 24 30 -0.0162 -0.151 0.039 5.96 0.64 0.19 0.33 5.17 3320S 19 40 32.0 +50 24 03 -0.0146 -0.160 0.039 6.05 0.00 -.01 0.34 3330S 19 41 02.2 +09 58 06 +0.0230 +0.160 0.040 10.00 1.26 1.17 -- 3340S 19 44 31.6 +33 36 37 +0.0014 -0.445 0.049 4.99 0.47 0.00 - 3350S 19 48 37.9 +10 17 21 +0.0162 -0.138 0.047 5.11 0.55 0.07 0.29 -
3360S 19 51 18.2 -24 04 01 -0.0097 -0.412 0.073 6.18 1.02 0.94 -- 3370S 19 52 51.4 +06 16 50 +0.0029 -0.479 0.070 3.71 0.86 0.48 0.49 2.57 3380S 19 54 33.1 -12 41 44 -0.0056 -0.509 0.060 9.30 1.30 1.22 0.56 - 3390S 20 00 16.8 +03 11 01 -0.0062 +0.115 0.071 7.46 1.12 ---- 3400S 20 01 34.0 +29 45 44 +0.0521 -0.527 0.046 5.71 0.73 0.37 -
3410S 20 01 51.3 +16 56 00 -0.0277 -0.411 0.058 5.80 0.61 0.09 3420S 20 12 24.1 +77 04 50 +0.0270 +0.511 0.072 8.89 1.36 ------3430S 20 29 39.6 -10 01 31 +0.0205 +0.103 0.032 5.65 0.69 0.21 - 3440S 20 29 50.0 +65 16 36 +0.0710 +0.280 0.127 10.43 1.59 1.39 1.07 - 3450S 20 36 42.0 +09 54 32 +0.0215 +0.021 0.026 5.05 0.72 0.21 -
3460S 20 37 13.4 -23 57 29 +0.0360 +0.464 0.070 6.37 0.72 0.23 0.26 - 3470S 20 44 16.5 +61 38 39 +0.0128 +0.822 0.073 3.43 0.92 0.62 0.49 2.27 3480S 20 44 20.2 +15 56 35 -0.0024 -0.195 0.026 5.14 0.49 0.08 -- 3490S 21 00 53.2 +45 41 04 +0.0352 +0.149 0.048 7.68 0.97 0.78 -- 3500S 21 02 51.4 +06 52 36 +0.0054 -0.561 0.050 8.28 1.22 1.18 0.50 -
3510S 21 04 39.9 +38 29 59 +0.3523 +3.185 0.296 5.21 1.18 1.11 0.65 3.54 3520S 21 04 40.0 +38 30 00 +0.349 +3.20 0.296 6.03 1.37 1.23 0.83 4.03 3530S 21 09 40.0 +17 32 04 -0.0078 -0.893 ---- 7.41 0.50 ------3540S 21 14 05.4 +09 11 09 +0.0110 -0.123 0.068 7.95 1.02 0.84 0.40 3550S 21 17 25.0 -20 03 17 -0.0125 -0.724 0.049 9.16 1.35 1.26 0.60 29
HAO # SPEC RV HK W # BS # HD # SAO # BD # FIND CHART BIN
3160S 5 M2e - 3.0 5.105 735 3170S 5 GO -47.2 0.180 738A 7162 176051 67612 +32 3267 0 3180S 5 M2 +18.8 1.500 740 - 176029 124104 +05 3993 102G022-10 3190S 4 F5 - 9.0 0.200 7163 176095 124112 +06 3989 3200S 5 F8 +16.0 7172 176303 104308 +13 3841 0
3210S 6 M2 +34.0 745B 132G184-49 Y 3220S 5 F2 - 4.0 9649 7312 180777 9341 +76 0717 3230S 5 M3 e +34.0 1.251 752A - 180617 ---- +04 4048 102G022-22 O 3240S 5 F6 -20.0 0.210 -- 7354 182101 124564 +09 4081 3250S 5 KO -20.5 0.155 758 7368 182488 68239 +32 3411 ------
3260S 4G8 -99.8 0.160 759 7373 182572 104807 +11 3833 Y 3270S 5 M1 -51.6 1.052 763 ---- 184489 124806 +04 4157 102G023-05 3280S 5 KO +26.7 0.222 764 7462 185144 18396 +69 1053 ------r Y 3290S 4 F5 -28.0 765A 7469 185395 31815 +49 3062 0 3300S 4 F3 -38.0 ------7460 185124 143621 -04 4861
3310S 5G3 -26 7503 186408 31898 +50 2847 0 3320S 5 G4 -27 7504 186427 31899 +50 2848 0 3330S 5 MO - 7.1 0.825 9667 G142-47 3340S 5 F5 + 4.7 0.150 9670A 7534 187013 68827 +33 3587 ------r 0 3350S 5 F8 - 0.1 0.150 9671A 7560 187691 105338 +10 4073 ------0
3360S 5 K5 - 7.1 770 7578 188088 188692 -24 15668 0 3370S 4G8 -39.8 0.141 771A 7602 188512 125235 +06 4357 0 3380S 5 Ml +3.1 773 - 188807 163135 -12 5594 3390S 5 K4 e -31.3 0.780 775 - 190007 125379 +02 4076 3400S 4 G6 -46.2 0.155 9683 7670 190360 88133 +29 3872 C
3410S 5G1 + 4.2 0.190 779 7672 190406 105635 +16 4121 0 3420S 5 MO - 2.0 0.878 786 - 193202 9679 +76 0785 3430S 4 G2.5 + 9.0 0.130 792.1 7845 195564 163665 -10 5423 C 3440S 5 M3 +24.0 1.964 793 U 3450S 4 G5 p -52.0 7896 196755 126059 +09 4600 0
3460S 5G8 -45.3 -- 796 7898 196761 189549 -24 16193 3470S 4 KO e -87.3 ---.- 807 7957 198149 19019 +61 2050 Y 3480S 5F7 - 7.0 7947 197963 106476 +15 4255 0 3490S 5 K3 -12.0 0.673 9717A - 200560 50388 +45 3371 G212-17 0 3500S 5 K6 -62.9 0.782 818 - 200779 126533 +06 4741 102G025-16
3510S 5 K5 e -64.3 0.605 820A 8085 201091 70919 +38 4343 0 3520S 5 K7 e -63.5 0.980 820B 8086 201092 ------+38 4344 0 3530S 5 F9 - 201891 106908 +17 4519 3540S 5 K8 -13.7 0.760 824 - 202575 126671 +08 4638 3550S 5 K6 +21.1 9736 - 203040 190243 -20 6185 30
HAO # RA --- DEC PMa PMS PAR V B-V U-B R-I I
3560S 21 24 11.0 +03 31 12 -0.0050 -0.060 0.052 10.57 1.36 1.08 . 3570S 21 27 16.3 -12 43 35 +0.0699 -0.265 0.061 9.10 1.27 1.25 0.56 - 3580S 21 34 37.0 +39 14 00 -0.0160 -0.160 0.076 10.01 1.53 ------3590S 21 35 45.0 +27 29 54 +0.0320 -0.020 0.071 9.85 1.49 1.26 0.81 3600S 21 42 06.7 +14 32 37 +0.0183 -0.089 0.066 5.94 0.59 0.04 -
3610S 21 50 15.8 +28 33 31 -0.0046 -0.062 0.040 5.53 0.42 -. 13 - 3620S 21 58 32.5 +72 56 30 -0.0162 -0.154 0.033 5.03 0.44 - 3630S 21 59 39.0 +01 09 42 -0.0310 -0.260 0.105 9.17 1.47 1.26 0.76 3640S 22 24 04.7 +04 08 17 +0.0200 +0.053 0.040 5.75 0.52 0.04 3650R 22 35 45.0 -15 35 30 +0.1600 +2.280 0.305 12.18 1.96 1.54 1.66
3660R 22 44 11.6 +11 54 57 +0.0159 -0.493 0.048. 4.19 0.50 -.03 0.31 3.45 3670R 22 48 24.7 +17 44 12 +0.0035 +0.014 3680R 22 49 51.9 +09 34 09 +0.0353 +0.049 0.041 5.16 0.48 -.01 -- 3690R 22 50 35.0 -14 31 12 +0.0640 -0.620 0.209 10.13 1.59 1.14 1.22 6.76 3700R 22 55 00.4 +20 30 01 +0.0145 +0.063 0.073 5.49 0.67 0.21 0.34 4.62
3710R 22 57 38.2 -22 47 38 -0.0658 +0.065 0.130 7.89 1.39 1.24 0.62 3720R 23 10 51.9 +56 53 31 +0.2530 +0.299 0.147 5.56 1.01 0.89 0.53 4.22 3730R 23 16 28.8 -13 43 38 +0.0210 -0.088 0.040 5.08 0.80 0.41 - 3740R 23 16 28.8 -13 43 38 +0.0210 -0.088 -- 7.60 0.91 0.67 -- 3750R 23 22 14.0 +57 35 00 -0.0010 -0.320 0.085 10.51 1.51 1.18 0.86 -
3760R 23 22 52.8 +23 07 43 +0.0140 +0.043 0.036 4.40 0.61 0.14 0.32 3.55 3770R 23 30 11.9 -17 07 09 +0.0218 -0.234 0.087 8.60 1.25 ---- 0.52 - 3780R 23 37 16.5 +77 21 12 -0.0198 +0.156 0.065 3.21 1.03 0.94 0.51 1.95 3790R 23 37 22.6 +05 21 19 +0.0251 -0.432 0.071 4.13 0.51 0.00 0.31 3.38 3800R 23 46 35.6 +02 08 12 +0.0656 -0.962 0.174 8.98 1.48 1.09 0.87 -
3810R 23 47 55.0 +30 04 30 +0.0190 +0.000 0.049 9.34 1.26 1.19 ---- 3820R 23 49 57.1 +75 15 57 +0.0824 +0.056 0.093 6.39 0.98 0.71 0.38 3830R 23 56 07.1 +46 27 03 +0.0548 -0.027 0.060 9.62 1.44 1.19 0.74 - 3840R 23 59 33.2 +26 49 03 +0.0628 -0.985 0.084 5.75 0.67 0.05 0.43 4.73 31
HAO # SPEC RV HK W BS# HD# SAO # BD # FIND CHART BIN
3560S 5 M1 + 2.0 0.938 9739 ------3570S 5 MO -86.7 -- 830 ---- 204587 164435 -13 5945 3580S 5 MO - 834A ------140G212-48 Y 3590S 5 MO e -13.3 1.553 835 ------+27 4102 132G188-09 0 3600S 5 GO e -18.9 0.323 9751 8314 206860 107364 +14 4668 102G026-31
3610S 4-5 F6 +19.0 0.155 -- 8354 207978 90065 +28 4215 3620S 5 F5 -21.0 ----- 8400 209369 10216 +72 1009 0 3630S 5 K8 e +20.3 1.534 846 ---- 209290 ------+00 4810 102G018-16 3640S 5 F5 -17.8 0.140 9782A 8548 212754 127529 +03 4705 0 3650R 5 M6 e -60.0 866 ------122G156-31
3660R 5 F7 -5.3 0.139 872A 8665 215648 108165 +11 4875 0 3670R 4 G5 p ------216219 108214 +17 4818 3680R 4 F7 +11.6 0.141 9801A 8697 216385 127810 +09 5122 C 3690R 5 M5 + 8.7 -- 876 ------15 6290 122G156-57 3700R 5 G4 -31.2 0.155 882 8729 217014 90896 +19 5036
3710R 5 M1 +16.6 -- 884 ---- 217357 191563 -23 17699 3720R 5 K3 -17.8 0.235 892 8832 219134 35236 +56 2966 A 3730R 4 G5 +10.0 0.168 894.2 8866 219834 165624 -14 6448 S 3740R 5 K2 +10.0 0.220 894.2 ---- 219834 ----- V 3750R 5 M2 e - 5.0 1.680 895 ------+57 2735 140G217-07
3760R 3 F8 p -11.0 0.269 8905 220657 91253 +22 4833 3770R 5 K5 e + 1.2 -- 898 - 221503 165756 -17 6769 0 3780R 4 Kl e -42.4 0.124 903 8974 222404 10818 +76 0928 3790R 5 F7 + 5.0 0.152 904 8969 222368 128310 +04 5035 0 3800R 5 M2 e -64.6 0.561 908 ------128397 +01 4774 102G029-68
3810R 5 K8 - 5.6 1.633 9841 ------+29 5007 G130-16 3820R 5 K3 + 1.2 -- 909A 9038 223778 10879 +74 1047 G242-42 S 3830R 5 MO + 4.5 1.945 913 ------53537 +45 4378 129G171-29 3840R 5 G2 -36.2 0.178 914A 9088 224930 91669 +26 4734 ------S 32 33
6. NOTES TO THE CATALOG 34
SOLAR STELLAR SPECTROPHOTOMETER CATALOG High Altitude Observatory - NCAR - Notes
HAO # NOTES
0 R Sun; MK
10 R Cpm with W #4, a=328"; Vys 216, ADS 48F; A m=1, A: 5K6, B: 5M0
20 R A: W #4, AB: a=158.6", A m=2.6; Ca II em (B); V?
30 R Shell Star
40 R CaII em, vel +0.7 km/s (3 plates RGO unpublished) Vys 84, V ?
50 R C=3, Vys 85, ADS 246, Mt Wilson: sdM 4e; AB: p=3020y, a=43.94", AC: 11.5V, a=34.6"; A: Ca II em (B), SB with 2K=26 (GCRV), B: H em (B), flare star (Haro 1968); MK
60 R V, also see notes for W #15 A
70 R G=Hyades; a=202.1", A m=5.4; CN=9 Cet OW; Prot=7.7
80 R Wolf 630 group; OW
90 R CN=14 Cet; OW
100 R G=61 Cyg, ADS 520; AB: P=25y, a=0.67", A m=0.2; OW
110 R CN=54 Psc; V ?, a=122.0", A m=4.9; OW; MK; Prot=48.0
120 R OW
130 R Call em (B)
140 R Vys 361
150 R CH subgiant (Sneden, 1983, PASP, p.745)
160 R V, a=181.2", A m=4.6; OW; Prot=38.0 35
HAO # NOTES
170 R C=8, companions C-H optical; ADS 671B, AB: P=480y, a=12.0", A m=3.8
180 R C=8, companions C-H optical; AB: P=480y, a=12.0", A m=3.8; A: P=9.209d, K=2.2 km/s, a sini=0.249, ADS 671, CN=24 q Cas; MK
190 R G=Sirius, UMa stream, V ?, CN=19 $2 Cet
200 R Call em (Dyer 1954); Vys 89
210 R C=5, AB: a=129.7", A m=5.5, C: BD# +60 0125, BC: 9.0V, A-BC: a=129"; A: P=127.951d, K=1.6 km/s, a sini=2.35, ADS 721
220 R Call em (B), cpm with W# 51, a=284"; Vys 2, suspected SB (Joy & Mitchell, Ap.J. 108, 234, 1948)
230 R Vys 365
240 R C=6, 5 visual, 1 astrometric; AB: a=0.83", A m > 3, P=18.5y; A: SB, P=8393d, K=2.8 km/s, a sini=308, CN=30 g Cas, SD
250 R AB: a=10" (LTT), Vys 367
260 R CN=44 And; OW; Prot=13.1
270 R C=2, a=49.8", A m=2.7, B: 5G7; CN=37 Cet
280 R
290 R C=4, AC: a=119.0", A m=6.6, AB: 11.7V 11.7V, a=2", CD: 10.4V, a=4.9" at 120" from A; G=Hyades, moving; SG, CN=48 o)And
300 R Discordant V and B-V: 6.96, +0.77 (Cape), 6.91, +0.87 (Eggen), 6.91, +0.90 (Warnner); a=336.0", A m=5.2
310 R OW
320 R C=3, both visual companions probably optical; AB: a=114.0", A m=8.4, P=197.9d, K=1.8 km/s, a sini=4.79, CN=50 v And 36
HAO # NOTES
330 R G=Hyades, P=20y, a=0.12", A m=3-4 V, companion 25% solar mass; MK
340 R V ?, G=Sco-Cen assoc., C=3, AB: a=19.0", A m=6.4, CN=107 Psc; OW
350 R Vys 381
360 R a=89.8", A m=9.5; OW, Peculiar
370 R CN=109 Psc
380 R Iron rich star, A: astrometric binary unresolved by speckle interferometry; a=91.1", A m=3.1
390 R CaII em (B); Vys 4
400 R C=2, a=30.0", A m=4.0
410 R The absolute magnitude 2.7 by Oke indicates that it might be a subgiant; CN=112 Psc; OW, SG
420 R
430 R CN=64 Cet; OW
440 R C=2, AB: a=36.2", A m=1.9, B: BD# +66 0193
450 R ADS 1739, RV double line spectra, orbit determined; G= C Her, a=65.4", A m=8.5, P=10.021d, K=9.4 km/s, a sini=1.30, CN=8 8 Tri
460 R Orbit determined, P=93.50d, K=19.4 km/s, a sini=22.3; SG
470 R Call em (B); Vys 96, RV star?
480 R CN= c For
490 R CN=76 a Cet; SG
500 R C=3, AB: a=165", 11.7V, B=dM5, AC: a=2", A m > 5, P=50y, unresolved by speckle interferometry; OW, dwarf ? Prot=45.0
510 R OW, Prot=5.7 37
HAO # NOTES
520 R G=Hyades, Call em, vel +48.8 km/s (RGO unpublished)
530 R ADS 2081, C=3, AB: a=22.3", A m=5.6, P=2720y, B: Ca II em (B), C: probably optical; CN=13 0 Per
540 R Orbit determined, P=958d, K=3.0 km/s, a sini=35.3, CN=1 1 Eri
550 R
560 R Canl em (B); V ?; OW; Prot=6.6
570 R RV single line spectra, orbit determined, P=3507d, K=6.7 km/s, a sini=308, unresolved by speckle interferometry, CN=46 p3 Ari, OW
580 R Vys 98
590 R G=Mel 20 #44, but not cluster member, Per OB3, a=146.2", A m=8.2, CN=t Per; MK
600 R SD
610 R ADS 2406; C=2, a=3.2", A m=6.4, CN=94 Cet
620 R Call em (B); Amp 0.10 IR, C=3, AB: a=268.7" A m=4.5, C: 11.9V, a=251"; OW, CN=96, iK1 Cet; Prot=9.4
630 R
640 R G=Hyades; Vys 101.
650 R CaII em (B); P=25y, a=2.0", A m=3.0, unresolved by speckle interferometry, CN=18 eEri; OW; MK; Prot=11.3
660 R OW
670 R CPM ? a-396.0", A m=10.0, CN=10 Tau
680 R Vys 427, V=9.72 (Eggen) or 9.58 (Mumford) Peculiar
690 R Canl em (B); Composition discussed by Hazelhurst (Observatory 83, 128, 1963); V? CN=23 6 Eri; OW 38
HAO # NOTES
700 R C=3, A-BC: a=17", 10.6V; MK
710 R CN=27 t 6 Eri
720 R Vys 434
730 R
740 R C=3, ADS 2894, A: Cal em (B), AB: a=ll.l", B: H em (B)
750 R Abundance analysis (Pagel and Powell 1966, R. Obs. Bull., No 124) Fe/H = 20 x solar value for this high velocity sub dwarf (Krishna Swamy 1968, ApJ. 154, 983); SD
760 R
770 R V ?, C=3, AB: a=170.1", A m=2.7; G=Hyades ?; CN=39 Tau
780 R Cpm with Yale 907=ADS2995: 7.3, dK2, 9.0; G=Hyades, OW, CN=50 Per; Prot=2.6
790 R V ?, cpm with HAO#800, C=4, AB: a=64.7", A m=0.6, OW; Prot=7.2
800 R Cpm with HAO#790, C=4, AB: a=64.7", A m=0.6, OW
810 R ADS 3090, C=5, A: CaII em (B), AB: a=83", A m=5, B: white dwarf, BC: a=6.9", var=DY Eri, C: 11.18V, dM4e, P=252.1y, other comparions optical; OW, CN=40 o2 Eri
820 R C=5, AB: a=83", A m=5, BC: 6.9", var=DY, Eri, WD
830 R C=5, BC: a=6.9", P=252.1y, var=DY Eri
840 R CaII em (B); Vys 8, objective prism classification K7II (Abastumani Bull. 35, 68, 1966). Probably variable: amplitude of observed differences: 1M (Petit. Inf. Bull. IAU 320, 1968)
850 R Weak Can em (Cowley, Hiltner and Witt 1967); Vys 449; MK
860 R SG 39
HAO # NOTES
870 R This star has intense H & K emission. Balmer lines cannot be detected, suggesting that they are filled in with emission. Other spectral lines are much broader than normal at this spectral type (Jones 1966, R. Obs. Bull. No 126); MK
880 R OW
890 R CaII em (B); Vys 107
900 R CN=58 Eri; OW; Prot=7.6
910 R G=Hyades?, ADS 3321, a=30.4", A: var in V (0.79 to 0.95); CN=-- Cep; SG
920 R Also classified G5V; G=H II 674; Classified on obj. prism plate G5V; SG; MK
930 R OW
940 R Vys 113, V ?, (suspected by Joy and Mitchell, ApJ. 108, 234, 1948)
950 R G=Sco - Cen assoc.; CN=68 Eri
960 R G=Hyades, moving; SG
970 R OW
980 R ADS 3864, C=3, AB: a=10.4", A m=3.7, B: 9.2V, 5 F6, BD# +79 0168
990 R G= e Ind; ADS 3886; C=6, B: 13.4V, a=29.1", C: 12.1V, a=42", D: optical, AD: a=146.6", A m=4.9, CN=15 X Aur
1000R ADS 3900; C=3, AB: a=2.7" (1960), AC: 10.4V, a=196.7"
1010R Vys 462; Cpm, RV, common parallax with HAO# 1020; a=12", CaII em (B)
1020R Cpm, RV, common parallax with HAO#1010; CaII em(B) C=2, a=85.7", A m=2.9; OW; CN=111 Tau
1030R Vys 463, G= y Leo
1040R Strong CaII em (Cowley, Hiltner, and Witt 1967); Vys 9; MK 40
HAO # NOTES
1050R Vys 464
1060R C=5, cpm with HAO#1070, a=99", Cal em (B); B: 9.8V, dM2, AD: a=688.0", A m=2.8
1070R Vys 465, cpm with HAO#1060, a=99"; Ca II em (B)
1080R CaII em (B); Vys 466; Peculiar
1090R G=Sirius, UMa, C=4, AB: a=96.5", A m=2.5, cpm with HAO# 1100
1100R G=Sirius, UMa, C=4, AB: a=96.5", A m=2.5, cpm, AC: a=18.7", AD: a=45", ADS 4334; CN=13 y Lep
1110R GOriOB I; SG
1120R G=Sirius, UMa, UMa stream; C=3, Occultation double with dia.=.0016", a=0.6", magnitude unknown, OW, CN=54 X1 Ori; MK; Prot=5.2
1130R CN=16 rlLep
1140R Call em (B); V=7.23 by Eggen. Argue gives 6.76 (M.N. 133, 475, 1966); G= near H II 73
1150R Weak CaII em (Cowley, Hiltner and Witt 1967); Vys 471
1160R C=3, AC: a=204.0", A m=4.2; BD# +12 1086, AB: 12.5V, a=24"; CN=74 Ori
1170R C=4, AB: a=189.7", A m=3.9; OW
1180R OW, R-I calculated by Eggen
1190S
1200S Vys 478
1210S 8 Sct?, v sini=70
1220S ADS 5425, B: 8.4m, orange; v sini < 6, A m=3.4, a=36.2", CN=56 V5 Aur
1230S Vys 479, Peculiar 41
HAO # NOTES
1240S Vys 239
1250S AB: A m=3.8, a=58.3"; ultraviolet deficient; B: 10.11V, +1.50 B-V, +0.93 R-I (Eggen), Spec=dM
1260S Vys 482, AC +33 25644
1270S ADS 55598, SB, C=2, AB: P3190y, a=9.550"; AC: a=1ll", 10.3V
1280S CN=37 Gem, v sini < 3
1290S CaII em, vel +16 km/s (FDS I); G=H I 117
1300S H em (B), V ? (Petit 1961), G=Hyades; C=2, RV range 110 km/s, AC+38 236216, +39 26259; MK
1310S v sini < 6, SG
1320S Vys 880, Cpm with W #274, a=12.6"
1330S C=2, Vys 17, Luyten's star, suspected astrometric binary; Unseen cp van de Kamp 1969, PASP. 81, 5
1340S Other classification 4 F7; v sini=0, G=C Her
1350S G=Hyades, cpm, B=13.2, sep=26", v sini=20
1360S ADS 6175A, 8 Sct?, v sini=6, SB, P=40.65y, K=1.7km/s, a sini=324, A m=10.3, sep=4.5", N: Procyon
1370S Vys 503
1380S A: CaII em (B), AB: a=58" (LIT)
1390S AB: a=58" (LTT)
1400S v sini < 10; CN=10 2t Cnc, SG; MK
1410S RV variable; MK
1420S CN=18 X Cnc, v sini=0
1430S Vys 254, unseen companion, C=2, P=25y, a=0.5", A m=3 (Lippincott, private communication 12/68) 42
HAO # NOTES
1440S G=Sirius; CN=3 n 1 UMa; G=Wolf 630, RV variable? v sini=4
1450S vsini=ll; OW
1460S Vys 531
1470S Lines of higher excitation potential show higher RV. G=Hyades, A: strong metallic line star with enhanced CN, C2 and perhaps CH; AB: a=85" (LTT), A m=7.0, cpm; B: HR 3521, magnetic star, 6.23-6.37V: CN=55 p1 Cnc
1480S Vys 532A, ADS 7067A, AB: orbits uncertain, P=1200y or 900y, a=7.508" or 6.234"; V (AB)= 8.03 (Rabe, Veroff, Stw. Muchen 6, Nr. 4, 1961)
1490S RV variable, v sini < 6; OW; MK
1500S RV variable, v sini=0; SG
1510S Spec type = 5 GO e; G=Hyades, v sini=5, OW
1520S Vys 541, ADS 7251A, G=Hyades; AB: Strong CaII em (Cowley, Hiltner, and Witt 1967); orbits P=1555.1y a=22.362" (Hopmann, 1954) P=687.0y, a=16.52" (Guntzel-Lingner 1955)
1530S See comments HAO #1520; ADS 7251B
1540S Vys 543, CanI em (B)
1550S A component with HAO# 1560, C=2, CN=31 T1 Hya, AB: a=6.57", A m=3.0; RV variable?, v sini=28
1560S C=2, AB: a=65.7", A m=3.0; RV variable, v sini=28; B component with HAO# 1550
1570S Faint CaII em (Cowley, Hiltner and Witt 1967)
1580S
1590S ADS 7441A, A: CaII em (B); AB: a=5.8" (1905) to 2.0" (1937), B not seen 1941-1958 (van Biesbroeck); RV variable, A m=8.5; CN=11 LMi, OW; Prot=18.1
1600S Vys 270, CaII em (B) 43
HAO # NOTES
1610S RV variable?
1620S Vys 552
1630S CN=15 LMi, v sini=3; MK
1640S Vys 558, RV star?, Peculiar
1650S Vys 121
1660S C=2, CN=20 LMi; v sini=3, A m=3.2, a=407", B=BD +32 1968, faint; MK
1670S G=old disc population; C=3, Spec also dM0, dK7; Var NSV 4765, microvariable in V, 6.59-6.66V; AB: A m=2.2, a=165.4"; B: BD +50 1724, 9.0V, PM -1.352; -.529"; C: BD +50 1723, 10.1V at a=303.5" from B; strong Cal em (Cowley, Hiltner and Witt 1967)
1680S Vys 569, uncertain binary pair, a=25", A m=lm (Worley 1962a)
1690S RV variable?, v sini=ll; OW
1700S C=2, CN=35 Leo, v sini=6; SG; MK
1710S Vys 574, UV Ceti flare star, H em (B), radio flares detected (Lovell 1964). Suspected double from variable pm; P=26.5y, a=0.110" (Reuyl 1943); CN=AD Leo
1720S Mag var? ( CSVS); RV var?, v sini=16, 8 Sct? amp. 0.02V
1730S RV variable, v sini=8; OW; Prot=12.3
1740S This star was deleted after the HAO numbers were assigned.
1750S Vys 127
1760S Vys 30, RV var, CaII em, vel +6.8 km/s (RGO unpub- lished); triple system with BD #57 1266 and W 395 (Worley 1962a)
1770S C=3, v sini=0, G=36 UMa A; AC: A m=3.4, a=139"; AB: a=120"; B: BD +56 1458; C: BD +57 1266; B & C: A m oc 5
1780S Vys 32 44
HAO # NOTES
1790S v sini=14, c=4, A m=4.0, a=124.5", B: optical, var: amp. 0.2V; mag var? (CSVS)
1800S RV variable?, v sini < 3, CN=47 UMa; MK
1810S AC +23 46846, AC +24 185-54 (both given), Vys 128
1820S Vys 129, Canl em and H em (Dyer 1954)
1830S Vys 594, CaII em (B), unseen companion, P=8y (Van de Kamp 1969); semi-axis major of the photocentric orbit a=0.0336", A m > 3, (Lippincott 1960); OW; MK; Prot=48.0
1840S Vys 35; AB: a=28" (LTT); A: CaII em (B); B: H em, flare star (Haro 1968); CN=WX UMa
1850S Vys 600, ADS 8083A; A: Weak CaII em (Cowley, Hiltner and Witt 1967); AB: a=36.6" (1844) to 34.9" (1960); to 34.8" (1962). Discussion of system by Hopmann 1959
1860S v sini < 6, C=4, A m=1.6, a=138.7"; Spec type 5 GO would give parallax of 0.043" but classified as sd F9, the star may be nearer than 20 pc; OW; Prot=7.6
1870S Vys 604
1880S Vys 603, ADS 8100A, optical, AB: a=7.0" (1965); cp=ADS 8100 B: a=9.9" (1831) to 36.2" (1940), 8.2V
1890S Vys 607
1900S Vys 38, V variable, UV Cet flare star possible; CN=SZ UMa
1910S ADS 8162A, RV var? C=3; A: metal rich dwarf with high iron abundance; AB: physical a=28.7" (1958), A m=l.1, both UV deficient; P=2000y, a=40.76"; B: 7.57V, 4-5 K2, C: 9.9V at a=90" probably physical; CN=83 Leo
1920S ADS 8162B, see HAO# 1910
1930S ADS 8196A, C=2, CN=88 Leo, v sini < 10, A m=2.8, a=15.5", P=5500y, circular orbit; B: ADS 8196B, RV -10 km/s, 4 K6; OW; Prot=14.0 45
HAO # NOTES
1940S RV variable?, v sini=14, CN=89 Leo; OW
1950S Call em (B); CN=61 UMa; C=2, A m=4.9, a=159.3", RV variable, v sini=17; OW; MK; Prot=17.1
1960S Vys 617
1970S Vys 286
1980S RV variable, C=3, AC: A m=5.0, a=512.3", v sini=3; CN=5 P Vir
1990S N: Groombridge 1830, RV var; AB: A m=5.5, a=1.7"; B: UV? 8.5-12V; CN=CF UMa, OW, SD
2000S Other spec type classification 4 KO
2010S RV variable, G=Arcturus, v sini=8, A m=6.8, a=73.3"; OW
2020S RV variable, v sini=8, G=Mel 111 #66 (Coma); OW; CN=9 Com
2030S Vys 649, CaII em (B)
2040S v sini < 3, var: amp. 0.05V; P=2429.9d, K=2.6 km/s, a sini=75.7, unresolved by speckle interferometry. Probable nearby star; CN=8 P CVn; MK
2050S Vys 670
2060S
2070S Vys 675, CaII em (B); RV var?
2080S C=2, Vys 298, AB: a=17" (Giclas 1964), Call and H em, exceptionally strong (Dyer 1954)
2090S G=61 Cyg, Vys 43
2100S Vys 141, ADS 8778A; AB: a=1.0" (1962), definite orbital motion (van Biesbroeck 1954); V (AB)=9.43, magnitude estimates of B: 13.2 and 14.9
2110S Vys 299 46
HAO # NOTES
2120S ADS 8804A, RV var? v sini=28, A m=0.1, physical a=0.2", C=3; AB: P=25.87y, a=0.662"; A: 5.05, F5V; B: 5.08, F5V, HR 4969; Color and spectrum for combined light. Var. of combined light not confirmed but 90 degree inclination of orbit indicates eclipse possible; CN=42 a Corn, OW; Prot=3.0
2130S Var? v sini=15, AD: A m=5.0, a=235.0" C-4, B: 12.5V at a=79"; C: a=184" discovered by John Herschel in 1897, not seen 1908 or later, CN=53 Vir, SG
2140S C=2, SB (5 or more years?), v sini=6, A m=5.8, a=90.8", B: visual companion is optical; OW, CN=43 P Com; Prot=12.4
2150S G=y Leo, RV variable, CN=57 Vir
2160S RV variable? v sini=7, A m=9.1, a=34.3", CN=59 Vir; OW
2170S ADS 8841AB, Spec: K1V + M1V, C=3; AB: 1.3" (1881) to 6.4" (1959); common motion (G); V joint: B: CaII em moderately strong (B), 10.2V; C: 10.5V at a=92"; OW; Prot=18.8
2180S CN=61 Vir, v sini < 17, A m=5.5, a=231.5"; OW
2190S Vys 46, ADS 8861AB, C=3; AB: a=17.3"; AC: a=52.6"; C: 12.3V
2200S RV variable, v sini=l, A m=3.6, a=286.4"; CN=70 Vir; MK
2210S Vys 143, Possibly smaller perturbation in RA with a period of between 15 and 20y (Bieger, AJ, 69, 804, 1964)
2220S Vys 692
2230S Vys 145, Call and Balmer em (Dyer 1954); CN=EQ Vir
2240S Vys 308, moderate Call em (Cowley, Hiltner, Witt 1967); G=y Leo, spectral variations observed (Kandel, Comptes Rendus 255, 1275, 1962) 47
HAO # NOTES
2250S ADS 9025A, AB: a=10.3" (1849) to 5.4" (1958); RV variable, v sini=14, A m=7.5, 8 Set?, 4.40-4.58V, P = several centuries, B: M2; CN=4 T Boo, OW
2260S G=61 Cyg
2270S v sini < 19, G=probable Hyades, CN=89 Vir
2280S Vys 702, Peculiar
2290S P=494.173d, K=8.42 km/s (Bertiau 1957), v sini=13, A m=6.0, a=112.6", a sini=55.1, un- unresolved by speckle interferometry, CN=8 Tr Boo; MK
2300S SB, A; P=12.4y, the half-shift in the astrometric orbit is 0.15" (Wagman, AJ, 54, 138, 1949)
2310S Orbit determined, P=726.6d, K=2.9 km/s, a sini=24.2, unresolved by speckle interferometry; OW, CN=14 Boo
2320S V var: 4.06 - 4.11, G=Wolf 630, CN=99 t Vir; OW; Prot=7.6
2330S Vys 715, Peculiar
2340S Vys 312, photometry by Eggen, Cowley, Hiltner, and Witt give 8.57, +1.29, +1.20; Weak CalI em (Cowley Hiltner and Witt 1967)
2350S RV variable, v sini=l; OW
2360S C=3, AB: a=69.2", A m=7.0 (1854-1918) C: approximately cpm with AB, north of AB 1.5 degrees; parallax of AB used for C; CN=23 O Boo
2370S ADS 9273 AB; C=3; AB: a=4.8" (1829-1958), A m=3.9; B: 9.7V, 5G4, RV= -8V km/s; cp: 12.6V, a=92.8"; CN=105 $ Vir, SG; MK
2380S Vys 719; cpl: a=50", A m=0.6, cp2: uncertain, A m=3
2390S G=Hyades
2400S 48
HAO # NOTES
2410S Vys 722
2420S G=61 Cyg
2430S ADS 9413 AB, G=UMa stream, C=4, v sini=3, A & B: Call em (B), AB: A m=2.1, physical, a=7.2", P=151.505y, a=4.904"; masses 0.89 and 0.74 solar, perturbation period 2.2y, a=0.020" suspected, unresolved by speckle interferometry; B: 5K4, 6.9V, C: optical, 12.6V, a=282", cpm: invisible, P=10.2y; CN=36 , Boo, OW; Prot=6.2
2440S ADS 9413B, See HAO# 2430, OW; Prot=11.5
2450S Vys 726 B, ADS 94463, C=2, A: CaII em, vel +28km/s (FDS VI); AB: a=10.8" (1823) to 21.8" (1959); to 22.0" (1961). Uncertain hyperbolic orbit by Hopmann
2460S Vys 726A, ADS 9446AB, C=6, UV deficient, RV variable A: CaII em; AB: a=22.0" (1961); A m=2.3, hyperbolic orbit (Hopmann 1966); B: 5M2, 7.93V
2470S SG; RV variable? v sini=6
2480S Vys 55
2490S Vys 314
2500S G=Sirius, UMa stream; RV var, v sini=45, AC: A m=4.9; a=244.1", C=3, both optical, CN=45 Boo
2510S v sini < 6
2520S RV variable, v sini=2, CN=5 Ser, AB: A m=4.6 a=11.2", C=4; OW
2530S Vys 58
2540S v sini=0, SB: orbit determined, P=226.95d, K=14.0, a sini=32.0, unresolved by speckle interferometry; CN=31 e Lib, OW
2550S ADS 9716C, LTT 14639, W #593 physically connected, a=121" AB: P=55.88y, a=0.785", V (AB)=6.79; C: cpm and parallax with AB 49
HAO # NOTES
2560S Subdwarf
2570S LTT 14677, SB: orbit determined P=1837d, K=2.8, a sini=59.1, v sini < 6; CN=28 X Ser, OW; MK; Prot=18.0
2580S v sini < 17, A m=6.7, a=134.6"; CN=1 c CrB, SG; MK
2590S Spec: F 8V, Fe -2, H 8 -1; v sini=0. Lithium to hydrogen ration 12 times solar, low metal content. Variable intrinsic polarization observed 8-74; CN=1 X Her, OW
2600S C=3 optical? RV var? v sini=8, AB: A m=6.6, a=201.5" C: Color excess E (B-V)= +0.03, CN=41 y Ser
2610S RV var, v sini=7, A m=3.2, a=89.6", optical; CN=15 p CrB, OW
2620S LTT 6411
2630S
2640S LTT 14816. Strong metallic line star with enhanced CN and C2 (Greenstein and Oinas 1968 ApJ Letters, 153, L91); CN=14 Her
2650S v sini=2, A m=7.7, a=25.8, optical; CN=18 Sco; MK
2660S Vys 162, A: moderate CaII em (Cowley, Hiltner and Witt 1967); RV var?, AB: a=64.0"; MK
2670S Vys 763; Peculiar
2680S Vys 766, LTT 14898
2690S Also BD -1 3220, CaII em weak (B); Spec 5K2, UV deficient; CN=12 Oph, OW; Prot=21.3
2700S LTT 14967
2710S R-I from Eggen; OW; Prot=ll.l
2720S C=3, UV, AB: P=1.72y, a=0.218", A=9.7V, B=9.7V, H em (B), flare star (Petit 1961), ultra- violet flares detected (MacConnell 1968 ApJ, 153, 313) see W #643, CN=V 1054 Oph 50
HAO # NOTES
2730S Vys 785, RV var?, R-I by Eggen
2740S Vys 787A, AB: a=186", common spatial motion and parallax 0.086" and 0.101", B: W #654, Vys 787B
2750S LTT 15050, v sini < 6, OW; Prot=7.6
2760S Vys 790A, ADS 10386A, C=2, AB: a=22.3" (1830) to 22.3" (1949)
2770S Vys 790B, ADS 10386B, C=2, AB: a=22.3" (1830) to 22.3" (1949)
2780S ADS 10417C, CaII em, vel +2 km/s (FDS I), C=5, Cpl, 2:ADS 10417 B/A, HD 155885/6, HR 6401/2, W 663 A m=0.0, a=7.30", OW; Prot=18.0
2790S LTT 6908, AB: a=2.7" (1931) to 3.7" (1959); A m=4.5, Spec 3-4 Fl, v sini=0; V (AB)=4.39, Spec of B uncertain; CN=40 4 Oph
2800S C=3, v sini=0, AB: A m=5.1, a=230", B: not cpm; optical, var: amp 0.4V; CN=72 Her
2810S Vys 794
2820S Gliese #673.1, G=Hyades, Spec A3m, A9mi, F2, v sini=59; CN=44 Oph
2830S v sini=8, OW
2840S Vys 321, CaII em (B), cp: a=10.1" (1960), 14V; probably optical (Worley 1962a)
2850S ADS 10598A, G=C Her, A: 5.97V, AB: P=46.08y, a=1.02", A m=0.1, physical, a=0.7", B: 6.07V, m sin3 i=1.05, a sini=1230, OW; MK
2860S RV var, v sink 10; OW
2870S Vys 169, AC+18 1453-48, AC+19 997-273; R-I by Kron, Eggen gives +0.82, Mumford B-V= +1.71; AB: P=24y, a=0.041" (Van de Kamp 1968)
2880S LTT 15233; R-I on Cousins system; OW; Prot=33.5
2890S Vys 323; MK 51
HAO # NOTES
2900S RV var? v sini < 10; CN=84 Her, OW
2910S ADS 10759B, cpm with HR 6636, v sini<- 25, A m=1.2, sep=30.2"
2920S C=4, ADS 10786A, G=Wolf 630, AB: a=34" (1955), ABC physical, v sini=20, A m=6.4, B: 10.3V, 5M4, BC: P=43.20y, a=1.360", CaII em (B), C: 10.8V, D: 11.2V, AD: a=256.1"; CN=86 B Her, MK
2930S vsini=ll, SG
2940S Vys 799, N=Barnard's star, possible unseen cp (van de Kamp 1969, ApJ, 74, 757)
2950S Vys 176, LIT 7180
2960S C=2, ADS 11046A, v sini=16, a sini=1300 AB; P=87.85y, a=4.55", SB, K=3.1 km/s, A m=1.8, physical a=1.9", A & B Call em (B), B: SB, 6.00V, 5K4, B-V=1.15, Aitken listed 9 additional companions within 180"; CN=70 Oph, OW; Prot=19.7
2970S C=3, Orbit determined, AB: A m=0.4, a=19.3", P=10.5217d, K=46.2 km/s, v sini < 25, m sin3 i=0.462, a sini=6.36, A=HR 6810; CN-40 Dra, SG
2980S C=3 v sini=0, AB: A m=0.4, a=19.3", B; HR #6809 C: faint at a=221.0"; CN=41 Dra, SG
2990S The large value of B-V does not fit the classification as a dwarf
3000S RV var? G=Wolf 630 group; OW; Prot=42.0
3010S LTT 15404, Gliese 708.1, v sini=8, CN=36 Dra
3020S LTT 7350
3030S LTT 7358, R-I by Eggen, Var: amp. 0.06V, G=IC 4725.26, HII 376
3040S Vys 181, LIT 7369
3050S v sini=14, SG 52
HAO # NOTES
3060S C=3, both companions optical, AC: v sini=55, A m=6.7, a=74.8"; SG
3070S
3080S C=2, Vys 184, ADS 11632A, P=453y, a=15.66"
3090S See comments for HAO#3080; ADS 11632B
3100S C=5, LTT 15529, cpl: a=48.2", 13V; cp2: a=63.8", l1V, cp3: a=12.6", 14V, cp4: a=37.6", 13.7V; Infrared, Var?, v sini=14, CN=110 Her
3110S Vys 805, LTT 7448; peculiar
3120S Vys 325, ADS 12696A, LTT 15535, optical cp: llm, a=12" (1829) to 58" (1962) G
3130S Vys 185
3140S Vys 186, LTT 15550, +16 247-80, +17 435-695 CaII em (B)
3150S RV var?, Luminosity class possibly brighter than main sequence; SG; MK
3160S Vys 188, AC +9 142-269, +8 142-393, CaI em and H em (Dyer 1954)
3170S ADS 11871A, LIT 15567, C=6, RV var, v sini=4, AB: P=61.2y, a=1.24", A m=2.2, physical a=0.7, B: 5K1; OW; MK
3180S Vys 190
3190S v sini< 10, OW
3200S G=UMa stream, v sini=26, C=3; AB: A m=4.3, a=17.8", optical. CN=11 Aql, SG
3210S C=2, LIT 15602, AB: a=115" (LTT); SD
3220S Gliese #748.1, G=Sirius; G=UMa stream, spec 5A9, v sini=63; CN=59 Dra
3230S Vys 65; A: Cal em (B); AB: a=74", B: flare star. van Biesbroeck's star, has lowest known luminosity 17.38V, B-V=2.12; MK 53
HAO # NOTES
3240S v sini=12, OW
3250S Spec 5G8
3260S C=3, G=61 Cyg, RV var, v sini < 17, AB: A m=3.5, a=105.6"; CN=31 Aql, OW; MK
3270S Vys 196
3280S v sini < 17, a=315.6", CN=61 a Dra; MK
3290S ADS 12695, LTT 15729, C=3; AB: a=4.2" (1934), cpm; B: 13V; C: 10.6V; AC: a=48.4" (1923), optical, A m=6.9; CN=13 0 Cyg
3300S RV var? CN=42 Aql, SG
3310S Binary with HAO #3320, v sini=2, MK
3320S Binary with HAO #3310, v sini=3, MK
3330S Vys 326, +9 148-85, LTT 15757
3340S ADS 12913A, LTT 15774, C=3, Gliese 767.1A, RV var?, v sini=9; AB: a=26" (1953), A m=3.5, pa=26.0, cpm with W #9669 AB, a=800"; B: 9.2-10.6V, 5K6; cp: ADS 12913C, AC: a=135" (1928) 9.0V, optical; CN=17 Cyg, OW
3350S ADS 13102A, LTT 15798, C=3, Gliese #768.1A, RV var?, v sini < 6; AB: A m=8.3, a=14.4", optical; B: ADS 13012B; C: 5M4, 13.8V; AC: a=22.5"; CN=54 o Aql, OW
3360S LTT 7861; SB, A m=4.0, a=31.5", optical
3370S ADS 13110A, LTT 15822, Var amp 0.05V, I, v sini < 16, C=3, AB: a=12.8" (1958), B: 12V, 5M3, AC: A m=7.7, a=175.0" (1925); CN=60 P Aql, OW; MK
3380S Vys 327, RV var
3390S CaII em (B); OW 54
HAO # NOTES
3400S Cpm with W #777, RV var, A m=9.8, a=179.0", iron rich star, cp: 16.4 pg, M6, OW
3410S C=6, RV var?, v sini=4, AC: A m=0.9, a=203.7"; CN=15 Sge, OW; Prot=13.5
3420S
3430S ADS 13960, RV var?, C=3, AB: a=4.6" (1878) and 4.4" (1943); cpm, B: 11.3V at a=3", AC: a=103.2"; SG; MK Woolley # 792.1A
3440S Vys 820, Ac +65 6955, uncertain binary pair, a=35", A m=2 (Worley 1962a)
3450S C=3, RV var, v sini < 19, AB: optical, B 11.8V at a=29", AC: cpm, C is 4K2, A m=4.8, a=203.6"; CN=7K Del, SG
3460S Mag var? (FDS VI) R-I by Eggen, RV var
3470S CaII em (B); v sini < 17, A m=8.2, a=51.7"; CN=3 il Cep
3480S G=Wolf 630, v sini < 25, binary with HR 7948, a=9.8", A m=1.0, P=3249y, physical a=13.813"; CN=12 y' Del, SG
3490S ADS 14585C, LTT 16160, C=5; AB: a=2.8" (1934) to 3.1" (1958) A =5.6; Cpl: a=17" (1908) to 3.9" (1958), 12.9V; Cp2 ADS 14585 AB=Yale 5064, 6.3V; Cp2-AB: a=165"
3500S Vys 831
3510S ADS 14636A, C=6, var?, v sini < 17; A:shows very weak and narrow central reversals (B); AB: Call em A m=0.8, a=28.7", P=653.34y a=24.307"; B: HAO#3520, 6.04V, 5K7. Astro- metric measures indicate 3 invisible cp at P=6, 7, 12y; unresolved by speckle interferometry. Suspected planetary companion not substantiated; CN=61 Cyg A, OW; Prot=37.9
3520S ADS 14636B, see comment for HAO#3510, v sini <-25, MK, Prot=48.0, OW 55
HAO # NOTES
3530S SD
3540S Vys 833, LTT 16242; R-I by Eggen, Mumford gives 7.95, +1.12
3550S Vys 201, Gliese 826.1
3560S Vys 70, +3 2561-36
3570S Vys 202
3580S Vys 836, LTT 16316, AC +39 60670, AC +38 59914, +40 904-361; AB: a=2.7" (1959) and 2.5" (1963) V (AB)=10.01
3590S Vys 203, LTT 16320, unresolved astrometric binary (Bieger 1964), CaII em (Byer 1954); cp: a=7.9" (1965) to 8.5" (1966), 11.4V
3600S LTT 16357, Can em (B), Gliese 836.7, RV var? v sini=ll, Amp. 0.002V var. due to star spots? Period of rotation =24.90d; var. H&K em indicates chromospheric activity; OW; Prot=4.7
3610S RV var? v sini < 6; weak lines, no G-bands, metals indicate 5F4, H and K, late F; CN=15 Peg, OW
3620S RV var, v sini=26, A m=6.8, a=131.4", optical; CN=16 Cep, SG
3630S Vys 335; MK
3640S ADS 15935A, LTT 16573, C=3, RV var, v sini=7; AB: a=2.6" (1875) to 3.5" (1937); A m=6.5; B: K4, C: ADS 15935C, a=103" 12.8V; G=Hyades moving, CN=34 Peg, OW
3650R Very red; H and Cal em (Eggen and Greenstein 1965, Ap.J. 142, 925); L 789-6
3660R ADS 16261, C=3, G=Wolf 630, AB: a=11.8"; B: 12V, 5M1, AC: a=145", A m=7.5; CN=46 4 Peg
3670R CH subgiant (Sneden, 1983, PASP, 745)
3680R C=2, AB: a=248", A m=8.4, B: M4; OW; CN=49 a Peg 56
HAO # NOTES
3690R Vys 337, V=10.17 (Hi. Johnson) or 10.10 (Eggen)
3700R Also classified as 5G5, CN=51 Peg; OW; MK
3710R Vys 339
3720R Var amp. 0.02B; astrometric binary unresolved by speckle interferometry. C=2, AB: a=106.6", A m=3.8; MK
3730R ADS 16672, C=3, AB: a=13.0", A m=2.5, A: a=0.2", A m=2.4, P=2323.6d, K=5.5 km/s, a sini=175, B: HAO#3740, 5K2, CN=94 Aqr, Woolley # 894.2A
3740R ADS 16672, AB: a=13.4", CN=94 Aqr; OW; Prot=42.0, Woolley # 894.2B, companion to HAO# 3730
3750R CaI em (B), Vys 211
3760R G=Hyades moving; CN=68 v Peg; SG
3770R Vys 864, C=3 with HAO# 3770, and W# 897AB. W# 897AB: a=0.2", (1962), V=10.39
3780R CaII em (B); CN=35 y Cep
3790R V?, a=69.9", A m=8.7, CN=17 t Psc
3800R H em (B), Vys 82
3810R
3820R C=3, ADS 17062, AB: a=4.6", B: 12V, M2, A: P=7.7532d, K1=39.9, K2=49.7 km/s, a sini=4.25, AC: a=161.9", A m=1.9; MK
3830R G=Hyades, Vys 214
3840R C=4, ADS 17175, G=Sco-Cen assoc., AB: a=0.8", A m=3.0, P=26.4, K=5.1 km/s, a sini=622, B: 5K6, AC: a=75.5", A m=3.1, C=5 K7, OW, CN=85 Peg