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Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem

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Informazioni su questo libro Si tratta della copia digitale di un libro che per generazioni è stato conservata negli scaffali di una biblioteca prima di essere digitalizzato da Google nell’ambito del progetto volto a rendere disponibili online i libri di tutto il mondo. Ha sopravvissuto abbastanza per non essere più protetto dai diritti di copyright e diventare di pubblico dominio. Un libro di pubblico dominio è un libro che non è mai stato protetto dal copyright o i cui termini legali di copyright sono scaduti. La classificazione di un libro come di pubblico dominio può variare da paese a paese. I libri di pubblico dominio sono l’anello di congiunzione con il passato, rappresentano un patrimonio storico, culturale e di conoscenza spesso difficile da scoprire. Commenti, note e altre annotazioni a margine presenti nel volume originale compariranno in questo file, come testimonianza del lungo viaggio percorso dal libro, dall’editore originale alla biblioteca, per giungere fino a te. 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I criteri che stabiliscono se un libro è protetto da copyright variano da Paese a Paese e non possiamo offrire indicazioni se un determinato uso del libro è consentito. Non dare per scontato che poiché un libro compare in Google Ricerca Libri ciò significhi che può essere utilizzato in qualsiasi modo e in qualsiasi Paese del mondo. Le sanzioni per le violazioni del copyright possono essere molto severe. Informazioni su Google Ricerca Libri La missione di Google è organizzare le informazioni a livello mondiale e renderle universalmente accessibili e fruibili. Google Ricerca Libri aiuta i lettori a scoprire i libri di tutto il mondo e consente ad autori ed editori di raggiungere un pubblico più ampio. Puoi effettuare una ricerca sul Web nell’intero testo di questo libro da http://books.google.com 1 EPHEMERIDES ASTRONOMICAE Anni 1800 . AD MERIDIANUM MEDIOLANENSEM SUP PUT A TA E AB ANGELO DE CESARIS ROMANA ACCEDIT APPENDIwas la Cum observationibus & Opusimise FACOLTA O R. TA FISIG ! MEDIOLANI MDCCXCIX . APUD JOSEPH GALEATIUM TYPOGRAPHUM 16682 N Chic ; 15.1OU.Pric 50 V CECIL ! VVUCITO DS 12D312 * VI* و * ? VD LED : 7021 700TVZET.LV VII Izcoa ار فده : " SOSIDEO 3 ECLIPSES ANNI ' 1 800 .. un Aprilis " Eclipfis Lunæ 9 Mediolani inviſibilis > Luna nondum orta 2 Initium 3h43 meridie Finis oh 17 Quantitas eclipſis digit.oh so in limbo Lunæ Auſtralis su tilf izVD1 ! ) , 24 Aprilis Eclipſis Solis Mediolani inviſibilis , Sole in inferiore horizonte deliteſcente ? " Conjun & tio ih 6 à media nocte inni Latitudo Lunæ 33 ' ** Borealis . ce d 2 b & tobris Ecliplis Lunæ Mediolani viſībilis * ! Initium 9h37 a meridie Finis 3 11h 28 ' } Quantitas : : : digit . 2 ° 43 ' in limbó Lunæ Boreali 18 O tobris Eclipſis Solis Mediolani inviſibilis Conjunctiogh gh 48481 ' a media nocte Latitudo Luna 35 ' Auftralis HABENTUR IN APPENDICE . Cata Vatalogus Stellarum Mediolani viſibilium ad initium anni 1800. redactus juxta recentes obſervationes à Franciſco Reggio . Pag . 5 Tabula fa & torümi decimalium variationis annuæ ſtel . larum ad affequendam ejuſdem . variationis quanti tatem pro quavis anni die . 27 Tabula motus annui prporij ſtellarum 28 Tabula reductionis partium æquatoris ad partes tem poris fiderei 31 Tabula reductionis temporis fiderei ad partes æquatoris 33 Tabula accelerationis ſtellarum in tempore folari medio 33 Tabula partium æquatoris reſpondentium tempori horologii accurate ſequentis motum ſolarem me . dium , aut aberrantis ad quatuor uſque fecunda 34 Tabulæ generales aberrationis aſcens . rectæ , & decli nationis ftellarum conftruétæ aclar . de Lambre 38 Tabulæ generales nutationis aſcens . rectæ , & declina . tionis ſtellarum ſupputatæ in ellipſi a clar . Lambert 40 ufu Tabula tangentium , & fecantium naruralium pro præcedentium tabularum aberrationis , & putationis 42 Æquatio generalis meridici prodeuntis ex altitudini . bus correſpondentibus Solis . pag . 43 Tabula refractionum mediarum 45 Tabulæ denſitatis aeris ſuppoſita ' r , quæ refpondet altitudini barometri 28 pol . & thermometri + io so Differentiæ meridianorum inter obſervatorium Medio lanenſe , & alia terræ loca aſtronomicis . vel geo . deticis obſervationibus determinatz 53 Oppofitio Urani cum fole anni 1799 menſe martio obfer . 58 Obſervationes Angeli de Ceſaris 61 De æquationibus motus Martis ab attractione aliorum planetarum prodeuntibus ex Barnaba Oriani 65 Obſervationes meteorologicæ habitæ in Specula Me . diolanenſi anno 1797 a Franciſco Reggio • TOS .. F E ST A MOBILIĄ . Septuageſima 19 91 Februarii Dies Cinerum 26 Lis Pascha Resurrectionis ai 13 Aprilis Rogationes Ritu Romano 19 Ascenſio Domini 22 Maji Rogationes Riru " Ambroſiano 261 ) Pentecoftes 7.21 Li Dominica SS . Trinitatis 18 Junij Solemnitas Corporis Chrifti Adventus . Ritu Ambroliano 16 Novembris Adventus Ritu Romano 30 , Cyclorum Numeri . Numerus Aureus . 15 Indictio Romana . 3 Cyclus Solaris . 17 Litera Dominicalis E Epacta . IV | Litera Martyrologii d Quatuor Anni Tempora . Vere 5 7 8 Martii Æftate 4 6 7 Junji Autunno 17 19 20 Septembris Hyeme . 17 19 20 Decembris Obliquitas Eclipticæ apparens · 1 Januarii 23 ° 28 ' 0 ' ' , 6 1 Aprilis 23 28 0,7 1 Julii 23 28 0,8 > 1 O & tobris 23 28 O 29 JANUARIUS 1800 . Dies Dres Phenomena s Obſervationes Phenomena Observationes 1 Solis . , Lune . Sol in paralello . 2 Primus Quadrans 1Th28 ' s'y Leporis culmin . 108 29 ' ) slad 8 Arietis 11h 431 9'e Corvi culmin . 16h 57 ' s Apogea , 12 Sol in nodo Saturni . gad 12 ; Tauri gh srl 13 € Corvi culmin . 16h 16 : 0ad , Geminorum Ch91 164 Leporis culmin . 9h 24.10 Plenilunium 1 ; 2 47 ' 14 Leporis culmin . gh 43'11 sad 2 y Gancri ih jo ' 19 Sol in figno Aquarii 17h 343ad , Leonis 5h 24.3 55 ' Ceti culmin . 4h14 15 ad , Virginis h 18 " 18 Scorpii culmin . I9h 22416 ad y & Virginis , gh.36 ' & inal 290 Leporis culmin . gh 34 Ultims 13 Canis culmin . gh 23-11 Ouádrans 2ch 191 glad , Virginis tl 427 19 Perigea ad Libræ , 33 20hd & Scorpii 24 Novilunium ich 45 ' 27ad 1 2 3 Aquarii iki 23 ' , 136 13 ' , Ighali Planete in parallelis fixarum . Uranus i Orionis , c . Pifcium . Phenomena Obfervationes Saturnusy : Arietis ; & Tauri ; Planetarur . Arietis ; ; Cancri . Jupiter S ; H , Geminorum ; d Uranus ftat . S - Andromedæ . Venus ad , Libræ diff . lat . 47 Mars $ # Leporis ; $ Crateris ; Venus ad 8 Libre diff . lat . 15 Scorpii Hydre Chivi ; Mars ad w Ophiuci diff . lat . 23 y Leporis ; e , ! Navis Ca Mercurius ftát . nis ; a Corsi . 13 Mars in nodo , Venus in Canis ; & Corvi , Sirii ; 17 Mercurius in elongațioue inixi a Crateris ; 3 Hydia IZ ma mane . Leporis ... 14_B Scorpii ; 22 Mars ad § Ophiuci di !. lat . 47 B Ceti , 1 ,. 54 Eridanis B , 22 Vénus ad Opliuci diff . fat . 36 Leporis . 24 Mercurius ' ad " o Sagittarii diff . Mercurius 12 , 54 Eridani lat . ; but 46 ' Ophiuci ; 8 , ' s Leporis ; 6 Cra 25 Mercurius in nodo . teris ; Scorpii ; ? Eridani , 26 Saturnus in oppoſitione Soli . B Corvi ; é , Leporis . А II JANUARIUS 18co . hebdom menfis Dies Dies Æquatio 1 Diffe./ Longitudo Afcenfio LEGE Declinatio . addenda rentia Sulis recta Solis tempori Vero Solis Auſtralis ut habeatur medium " M. S. S. S. G. M. S. G. M. S G. M. S. I Merc . 4 1,3 28,3 9 10 54 54 23. I , 3 2 Jov . 4 29,6 9 II 56 27,9 282 58 34 22 55 49 3 Ven . 4 57,5 9 12 57 17 284 4 4 22 50 4. Sat. 525,0 27,5 9 27,0 13 58 28 285 10 43 2 % 43 58 5 Dom . 5 52,0 26,5 9 14 59 38 286 16 37 22 37 22 6 Lun . 6 18,5 26,0 9 16 O 48 -87 22 25 22 20 44,5 19 7 Mart . 6 917 I 57 288 8 5 22 22 49 8 Merc . 7 10,1 25,6 9 18 25,0 3 6 289 33 37 22 14 53 9. JOV . 7 35,1 9 19 4 IS 290 392 22 6 31 10 Ven . 7 , 59,5 24,4 9 20 23,8 5 23 291 44 18 21 57 42 Il Sat. 8 23,3 9 21 6 31 292 49 25 1 48 28 12 Dom 23,2 . 8 46,5 9 22 7 38 293 54 23 21 38 49 9 22,6 13 Lun . 9,1 22,0 9 23 8 45 294 59 12 128 45 14 Mart 9 31,1 . 21 4 9 24 9 51 296 351 21 18 16 15 Merc .
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    1. M. Platiša, M. Popović, M. Dimitrijević, N. Konjević: 1975, Z. Fur Natur- forsch. 30a, 212 [A 1].* 1. Griem, H. R.: 1975, Stark Broadening, Adv. Atom. Molec. Phys. 11, 331. 2. Platiša, M., Popović, M. V., Konjević, N.: 1975, Stark broadening of O II and O III lines, Astron. Astrophys. 45, 325. 3. Konjević, N., Wiese, W. L.: 1976, Experimental Stark widths and shifts for non-hydrogenic spectral lines of ionized atoms, J. Phys. Chem. Ref. Data 5, 259. 4. Hey, J. D.: 1977, On the Stark broadening of isolated lines of F (II) and Cl (III) by plasmas, JQSRT 18, 649. 5. Hey, J. D.: 1977, Estimates of Stark broadening of some Ar III and Ar IV lines, JQSRT 17, 729. 6. Hey, J. D.: Breger, P.: 1980, Stark broadening of isolated lines emitted by singly - ionized tin, JQSRT 23, 311. 7. Hey, J. D.: Breger, P.: 1981, Stark broadening of isolated ion lines by plas- mas: Application of theory, in Spectral Line Shapes I, ed. B. Wende, W. de Gruyter, 201. 8. Сыркин, М. И.: 1981, Расчеты электронного уширения спектральных линий в теории оптических свойств плазмы, Опт. Спектроск. 51, 778. 9. Wiese, W. L., Konjević, N.: 1982, Regularities and similarities in plasma broadened spectral line widths (Stark widths), JQSRT 28, 185. 10. Konjević, N., Pittman, T. P.: 1986, Stark broadening of spectral lines of ho- mologous, doubly ionized inert gases, JQSRT 35, 473. 11. Konjević, N., Pittman, T. P.: 1987, Stark broadening of spectral lines of ho- mologous, doubly - ionized inert gases, JQSRT 37, 311. 12. Бабин, С.
  • Downloads/ Astero2007.Pdf) and by Aerts Et Al (2010)

    Downloads/ Astero2007.Pdf) and by Aerts Et Al (2010)

    This work is protected by copyright and other intellectual property rights and duplication or sale of all or part is not permitted, except that material may be duplicated by you for research, private study, criticism/review or educational purposes. Electronic or print copies are for your own personal, non- commercial use and shall not be passed to any other individual. No quotation may be published without proper acknowledgement. For any other use, or to quote extensively from the work, permission must be obtained from the copyright holder/s. i Fundamental Properties of Solar-Type Eclipsing Binary Stars, and Kinematic Biases of Exoplanet Host Stars Richard J. Hutcheon Submitted in accordance with the requirements for the degree of Doctor of Philosophy. Research Institute: School of Environmental and Physical Sciences and Applied Mathematics. University of Keele June 2015 ii iii Abstract This thesis is in three parts: 1) a kinematical study of exoplanet host stars, 2) a study of the detached eclipsing binary V1094 Tau and 3) and observations of other eclipsing binaries. Part I investigates kinematical biases between two methods of detecting exoplanets; the ground based transit and radial velocity methods. Distances of the host stars from each method lie in almost non-overlapping groups. Samples of host stars from each group are selected. They are compared by means of matching comparison samples of stars not known to have exoplanets. The detection methods are found to introduce a negligible bias into the metallicities of the host stars but the ground based transit method introduces a median age bias of about -2 Gyr.