たて座ベータ星
出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2023/10/08 21:01 UTC 版)
たて座β星（たてざベータせい、β Scuti、β Sct）は、たて座にある連星である。年周視差に基づいて計算した、太陽からの距離は、およそ690光年である[3]。見かけの等級は4.22で、肉眼でみることができる[10]。
注釈
![{\displaystyle \log g[{\mbox{cgs}}]=0.94}](http://weblio.hs.llnwd.net/e7/img/dict/wkpja/https://wikimedia.org/api/rest_v1/media/math/render/svg/47f326250a45e14d753f4a246173fe3be58a025d)
出典
- ^ a b c d e f g h i j Griffin, R. E. (2008-02), “Spectroscopic binary orbits from photoelectric radial velocities - Paper 198: 48 Piscium, 16 Aurigae, 5 Herculis, and β Scuti”, Observatory 128: 21-56, Bibcode: 2008Obs...128...21G
- ^ a b c d e “bet Sct -- Spectroscopic binary”. SIMBAD. CDS. 2019年1月23日閲覧。
- ^ a b c d e f g Parsons, Sidney B.; Franz, Otto G.; Wassermann, Lawrence H. (2005-03), “The Fine Guidance Sensor Orbit of the G4 Bright Giant HD 173764”, Astronomical Journal 129 (3): 1700-1705, Bibcode: 2005AJ....129.1700P, doi:10.1086/427853
- ^ a b Hutter, D. J.; et al. (2016-11), “Surveying the Bright Stars by Optical Interferometry. I. A Search for Multiplicity among Stars of Spectral Types F-K”, Astrophysical Journal Supplement Series 227 (1): 4, arXiv:1609.05254, Bibcode: 2016ApJS..227....4H, doi:10.3847/0067-0049/227/1/4
- ^ a b Luck, R. Earle (1991-02), “Chemical abundances for cyanogen-weak giants”, Astrophysical Journal Supplement Series 75: 579-610, Bibcode: 1991ApJS...75..579L, doi:10.1086/191542
- ^ Pasquini, L.; de Medeiros, J. R.; Girardi, L. (2000-09), “Ca II activity and rotation in F-K evolved stars”, Astronomy & Astrophysics 361: 1011-1022, Bibcode: 2000A&A...361.1011P
- ^ a b Keenan, Philip C.; McNeil, Raymond C. (1989-10), “The Perkins catalog of revised MK types for the cooler stars”, Astrophysical Journal Supplement Series 71: 245-266, Bibcode: 1989ApJS...71..245K, doi:10.1086/191373
- ^ a b Parsons, Sidney B.; Ake, Thomas B. (1998-11), “Ultraviolet and Optical Studies of Binaries with Luminous Cool Primaries and Hot Companions. V. The Entire IUE Sample”, Astrophysical Journal Supplement Series 119 (1): 83-104, Bibcode: 1998ApJS..119...83P, doi:10.1086/313152
- ^ a b c Hünsch, M.; Reimers, D. (1993-09), “Circumstellar MG II Absorption in Ultraviolet Spectra of Hot Companions of Red Giants and the Meaning of the MG II Asymmetry Dividing Line”, Astronomy & Astrophysics 276 (1): 161-170, Bibcode: 1993A&A...276..161H
- ^ a b c Hoffleit, D.; Warren, W. H., Jr. (1995-11), “Bright Star Catalogue, 5th Revised Ed.”, VizieR On-line Data Catalog: V/50, Bibcode: 1995yCat.5050....0H
- ^ a b Wagman, Morton (1987-08), “Flamsteed's Missing Stars”, Journal for the History of Astronomy 18 (3): 209-223, Bibcode: 1987JHA....18..209W, doi:10.1177/002182868701800305
- ^ Bayer, Johann (1603), Ioannis Bayeri Rhainani I.C. Uranometria., Augustae Vindelicorum : Excudit Christophorus Mangus
- ^ 陳, 久金 (2005) (中国語), 中國星座神話, 台灣書房出版有限公司, ISBN 978-986-7332-25-7
- ^ “中國古代的星象系統 (63)： 斗宿天區” (中国語). AEEA 天文教育資訊網. 國立自然科學博物館 (2006年7月2日). 2019年1月25日閲覧。
- ^ Campbell, W. W.; Wright, W. H. (1900-11), “A list of nine stars whose velocities in the line of sight are variable”, Astrophysical Journal 12: 254-257, Bibcode: 1900ApJ....12..254C, doi:10.1086/140765
- ^ Young, R. K. (1927-01), “Three Long-Period Binary Orbits”, Journal of the Royal Astronomical Society of Canada 21: 35-37, Bibcode: 1927JRASC..21...35Y
- ^ Parsons, Sidney B. (1981-07-15), “Ultraviolet and optical studies of binaries with luminous cool primaries and hot companions. I - Intrinsic colors and newly recognized systems”, Astrophysical Journal 247: 560-568, Bibcode: 1981ApJ...247..560P, doi:10.1086/159066
- ^ Ginestet, N.; Carquillat, J. M.; Jaschek, C. (1999-02), “Spectral classifications in the near infrared of stars with composite spectra. III. Study of a sample of 137 objects with the Aurelie spectrograph”, Astronomy & Astrophysicsl Supplement 134: 473-482, Bibcode: 1999A&AS..134..473G, doi:10.1051/aas:1999444
[続きの解説]
「たて座ベータ星」の続きの解説一覧
- 1 たて座ベータ星とは
- 2 たて座ベータ星の概要
- 3 名称
- 4 関連項目
- たて座ベータ星のページへのリンク
