アンドロメダ座15番星
出典: フリー百科事典『ウィキペディア(Wikipedia)』 (2023/02/08 20:10 UTC 版)
アンドロメダ座15番星(アンドロメダざ15ばんせい、15 Andromedae、15 And)は、アンドロメダ座の恒星である。「アンドロメダ座15番星」という名称は、フラムスティード番号によるもので、アンドロメダ座V340星という変光星名も付与されている[3][1]。見かけの等級は5.56で、肉眼等級ではあるがだいぶ暗い[2]。年周視差を基に計算すると、太陽系から約252光年の距離にあるとみられる[3]。
注釈
出典
- ^ a b c d Samus, N. N.; et al. (2009-01), “General Catalogue of Variable Stars”, VizieR On-line Data Catalog: B/gcvs, Bibcode: 2009yCat....102025S
- ^ a b c Kharchenko, N. V. (2001-10), “All-sky compiled catalogue of 2.5 million stars”, Kinematika i Fizika Nebesnykh Tel 17 (5): 409-423, Bibcode: 2001KFNT...17..409K
- ^ a b c d e f g h “15 And -- Variable Star of delta Sct type”. SIMBAD. CDS. 2020年4月22日閲覧。
- ^ a b c d e f g Griffin, R. E.; Gray, R. O.; Corbally, C. J. (2012-11), “The composite-spectrum binary hypothesis does not explain the λ Bootis stars”, Astronomy & Astrophysics 547: A8, Bibcode: 2012A&A...547A...8G, doi:10.1051/0004-6361/201219112
- ^ a b c Iliev, Ilian Kh.; Barzova, Ina S. (1995-10), “Mass and age determination for 21 λ Bootis-type stars”, Astronomy & Astrophysics 302: 735-740, Bibcode: 1995A&A...302..735I
- ^ a b c d Draper, Z. H.; et al. (2016-02), “IR excesses around nearby Lambda Boo stars are caused by debris discs rather than ISM bow waves”, Monthly Notices of the Royal Astronomical Society 456 (1): 459-476, Bibcode: 2016MNRAS.456..459D, doi:10.1093/mnras/stv2696
- ^ a b c Su, K. Y. L.; et al. (2006-12), “Debris Disk Evolution around A Stars”, Astrophysical Journal 653 (1): 675-689, Bibcode: 2006ApJ...653..675S, doi:10.1086/508649
- ^ a b Murphy, Simon J.; et al. (2015-10), “An Evaluation of the Membership Probability of 212 λ Boo Stars. I. A Catalogue”, Publications of the Astronomical Society of Australia 32: e036, Bibcode: 2015PASA...32...36M, doi:10.1017/pasa.2015.34
- ^ a b c Cheng, Kwang-Ping; et al. (2016-04), “Utilizing Synthetic UV Spectra to Explore the Physical Basis for the Classification of Lambda Boötis Stars”, Astronomical Journal 151 (4): 105, Bibcode: 2016AJ....151..105C, doi:10.3847/0004-6256/151/4/105
- ^ Rufener, F.; Bartholdi, P. (1982-06), “List of 333 variable microvariable or suspected variable stars detected in the Geneva photometry”, Astronomy & Astrophysics Supplement Series 48: 503-511, Bibcode: 1982A&AS...48..503R
- ^ Abt, H. A. (1984), “Discovery of λ Bootis Stars”, in Garrison, R. F., The MK Process and Stellar Classification, p. 340, Bibcode: 1984mpsc.conf..340A
- ^ Gray, R. O. (1988-01), “The Spectral Classification of the λ Bootis Stars”, Astronomical Journal 95: 220-228, Bibcode: 1988AJ.....95..220G, doi:10.1086/114631
- ^ a b Paunzen, E.; Handler, G. (1996-03), “Pulsation of HD 83041 and HD 221756”, Information Bulletin on Variable Stars 4301: 1, Bibcode: 1996IBVS.4301....1P
- ^ Weiss, W. W.; et al. (1994-01), “The variable λ Bootis star HD 142994”, Astronomy & Astrophysics 281: 797-802, Bibcode: 1994A&A...281..797W
- ^ Dorokhova, T. N.; Dorokhov, N. I. (1997-02), “Observations of Three λ Bootis Stars by Using Dual Channel Photometer”, Information Bulletin on Variable Stars 4445: 1, Bibcode: 1997IBVS.4445....1D
- ^ Dorokhova, T. N.; et al. (2008-03), “The pulsating λ Bootis star 15 Andromedae: results from a three-site photometry campaign”, Astronomy & Astrophysics 480 (1): 187-191, Bibcode: 2008A&A...480..187D, doi:10.1051/0004-6361:20078750
- 1 アンドロメダ座15番星とは
- 2 アンドロメダ座15番星の概要
- 3 特徴
- 4 関連項目
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