ぎょしゃ座ラムダ星とは - わかりやすく解説 Weblio辞書

ぎょしゃ座ラムダ星

出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2024/04/20 21:52 UTC 版)

ぎょしゃ座λ星（ぎょしゃざラムダせい、λ Aurigae、λ Aur）は、ぎょしゃ座にあるソーラーアナログの恒星である^[9]。視等級は4.7で、肉眼でもみることができる^[1]。ガイア衛星が測定した年周視差に基づいて計算した地球からの距離は、40.7光年である^[2]。

脚注

注釈

^ ^a ^b パーセクは1 ÷ 年周視差（秒）より計算、光年は1÷年周視差（秒）×3.2615638より計算

出典

^ ^a ^b ^c ^d ESA (1997), The HIPPARCOS and TYCHO catalogues. Astrometric and photometric star catalogues derived from the ESA HIPPARCOS Space Astrometry Mission, ESA SP Series, 1200, Noordwijk, Netherlands: ESA Publications Division, Bibcode: 1997ESASP1200.....E, ISBN 9290923997
^ ^a ^b ^c ^d ^e ^f ^g ^h “lam Aur -- High proper-motion Star”. SIMBAD. CDS. 2018年6月16日閲覧。
^ ^a ^b ^c ^d ^e Holmberg, J.; Nordström, B.; Andersen, J. (2009-07), “The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics”, Astronomy & Astrophysics 501 (3): 941-947, arXiv:0811.3982, Bibcode: 2009A&A...501..941H, doi:10.1051/0004-6361/200811191
^ ^a ^b ^c ^d Millan-Gabet, R.; et al. (2011-06), “Exozodiacal Dust Levels for Nearby Main-sequence Stars: A Survey with the Keck Interferometer Nuller”, Astrophysical Journal 734 (1): 67, Bibcode: 2011ApJ...734...67M, doi:10.1088/0004-637X/734/1/67
^ ^a ^b ^c ^d Sitnova, T.; et al. (2015-08), “Systematic Non-LTE Study of the -2.6 < [Fe/H] < 0.2 F and G dwarfs in the Solar Neighborhood. I. Stellar Atmosphere Parameters”, Astrophysical Journal 808 (2): 148, Bibcode: 2015ApJ...808..148S, doi:10.1088/0004-637X/808/2/148
^ Valenti, Jeff A.; Fischer, Debra A. (2005-07), “Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs”, Astrophysical Journal Supplement Series 159 (1): 141-166, Bibcode: 2005ApJS..159..141V, doi:10.1086/430500
^ ^a ^b Gray, R. O.; et al. (2003-10), “Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I”, Astronomical Journal 126 (4): 2048-2059, Bibcode: 2003AJ....126.2048G, doi:10.1086/378365
^ 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
^ Greaves, J. S.; Wyatt, M. C.; Bryden, G. (2009-08), “Debris discs around nearby solar analogues”, Monthly Notices of the Royal Astronomical Society 397 (2): 757-762, arXiv:0907.3677, Bibcode: 2009MNRAS.397..757G, doi:10.1111/j.1365-2966.2009.15048.x
^ Lubin, Dan; Tytler, David; Kirkman, David (2012-03), “Frequency of Maunder Minimum Events in Solar-type Stars Inferred from Activity and Metallicity Observations”, Astrophysical Journal Letters 747 (2): L32, Bibcode: 2012ApJ...747L..32L, doi:10.1088/2041-8205/747/2/L32
^ Trilling, D. E.; et al. (2008-02), Astrophysical Journal, 674, pp. 1086-1105, Bibcode: 2008ApJ...674.1086T, doi:10.1086/525514
^ Eggen, O. J. (1971-06), “The ζ Herculis, σ Puppis, ε Indi, and η Cephei Groups of Old Disk Population Stars”, Publications of the Astronomical Society of the Pacific 83 (493): 251-270, Bibcode: 1971PASP...83..251E, doi:10.1086/129119
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^ Phillips, N. M.; et al. (2010-04), “Target selection for the SUNS and DEBRIS surveys for debris discs in the solar neighbourhood”, Monthly Notices of the Royal Astronomical Society 403 (3): 1089-1101, Bibcode: 2010MNRAS.403.1089P, doi:10.1111/j.1365-2966.2009.15641.x
^ Eggleton, P. P.; Tokovinin, A. A. (2008-09), “A catalogue of multiplicity among bright stellar systems”, Monthly Notices of the Royal Astronomical Society 389 (2): 869-879, Bibcode: 2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x
^ ^a ^b Allen, R. H. (1963), Star Names: Their Lore and Meaning, New York, NY: Dover Publications, Inc., p. 91, ISBN 0-486-21079-0 2018年6月15日閲覧。
^ Rhoads, Jack W. (1971-11-15), “A Reduced Star Catalog Containing 537 Named Stars”, NASA Technical Memorandum (Jet Propulsion Laboratory, California Institute of Technology): 11, 33-507
^ （中国語）陳, 久金 (2005). 中國星座神話. 台灣書房出版有限公司. ISBN 978-986-7332-25-7
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