格利泽908
![]() 格利泽908的可見光變曲線[1] | |
觀測資料 曆元 J2000 | |
---|---|
星座 | 雙魚座 |
星官 | |
赤經 | 23h 49m 12.52790s[2] |
赤緯 | 02° 24′ 04.4072″[2] |
視星等(V) | 8.93 - 9.03[3] |
特性 | |
光谱分类 | M1V Fe-1[4] |
变星类型 | BY Dra[3] |
天体测定 | |
徑向速度 (Rv) | 2998282099999999999♠−71.79[5] km/s |
自行 (μ) | 赤经:7002992665000000000♠992.665[5] mas/yr 赤纬:2997031351999999999♠−968.648[5] mas/yr |
视差 (π) | 169.2163 ± 0.0281[6] mas |
距离 | 19.275 ± 0.003 ly (5.9096 ± 0.0010 pc) |
绝对星等 (MV) | +10.1[7] |
詳細資料 | |
質量 | 0.37[8] M☉ |
半徑 | 0.39[9] R☉ |
表面重力 (log g) | 4.86[9] |
亮度 (bolometric) | 0.022[9] L☉ |
溫度 | 3,570[9] K |
金属量 [Fe/H] | 3000490000000000000♠−0.51±0.05[10] dex |
自轉速度 (v sin i) | 2.25[11] km/s |
其他命名 | |
參考資料庫 | |
SIMBAD | 资料 |
![]() ![]() Gliese 908 格利泽908在雙魚座的位置 |
格利泽908是一顆位於雙魚座的紅矮星,距離地球19.3光年。它是一顆天龍座BY型變星,變星編號為BR Piscium。由於星斑和不同的色球活動,它的視星等在8.93和9.03之間變化。
格利泽908的可變性在1994年得到確認,儘管其亮度變化沒有檢測到週期性。[16]1997年進入變星總表。[17]
格利泽908是一顆主序星,光譜等級為M1V Fe-1。後綴表示明顯缺乏重元素。[4]
參考
- ^ ASAS-SN Variable Stars Database. ASAS-SN Variable Stars Database. ASAS-SN. [6 January 2022]. (原始内容存档于2023-01-11).
- ^ 2.0 2.1 2.2 Perryman; et al. HIP 117473. The Hipparcos and Tycho Catalogues. 1997 [2023-03-21]. (原始内容存档于2016-03-04).
- ^ 3.0 3.1 Samus, N. N.; Durlevich, O. V.; et al. VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013). VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 2009, 1: B/gcvs. Bibcode:2009yCat....102025S.
- ^ 4.0 4.1 Keenan, Philip C.; McNeil, Raymond C. The Perkins Catalog of Revised MK Types for the Cooler Stars. The Astrophysical Journal Supplement Series. 1989, 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.
- ^ 5.0 5.1 5.2 Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; et al. Gaia Data Release 2. Summary of the contents and survey properties. Astronomy & Astrophysics. 2018. Bibcode:2018A&A...616A...1G. arXiv:1804.09365
. doi:10.1051/0004-6361/201833051. VizieR中此天体在盖亚望远镜第二批数据发布的记录
- ^ Brown, A. G. A.; et al. Gaia Early Data Release 3: Summary of the contents and survey properties. Astronomy & Astrophysics. 2021, 649: A1. Bibcode:2021A&A...649A...1G. S2CID 227254300. arXiv:2012.01533
. doi:10.1051/0004-6361/202039657
. 已忽略未知参数
|collaboration=
(帮助) (勘误: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR. - ^ Boro Saikia, S.; et al, Chromospheric activity catalogue of 4454 cool stars. Questioning the active branch of stellar activity cycles, Astronomy and Astrophysics, 2018, 616: A108, Bibcode:2018A&A...616A.108B, S2CID 118915212, arXiv:1803.11123
, doi:10.1051/0004-6361/201629518.
- ^ Perger, M.; García-Piquer, A.; Ribas, I.; Morales, J. C.; Affer, L.; Micela, G.; Damasso, M.; Suárez-Mascareño, A.; González-Hernández, J. I.; Rebolo, R.; Herrero, E.; Rosich, A.; Lafarga, M.; Bignamini, A.; Sozzetti, A.; Claudi, R.; Cosentino, R.; Molinari, E.; Maldonado, J.; Maggio, A.; Lanza, A. F.; Poretti, E.; Pagano, I.; Desidera, S.; Gratton, R.; Piotto, G.; Bonomo, A. S.; Martinez Fiorenzano, A. F.; Giacobbe, P.; et al. HADES RV Programme with HARPS-N at TNG. II. Data treatment and simulations. Astronomy and Astrophysics. 2017, 598: A26. Bibcode:2017A&A...598A..26P. S2CID 56341358. arXiv:1610.08698
. doi:10.1051/0004-6361/201628985.
- ^ 9.0 9.1 9.2 9.3 Maldonado, J.; Affer, L.; Micela, G.; Scandariato, G.; Damasso, M.; Stelzer, B.; Barbieri, M.; Bedin, L. R.; Biazzo, K.; Bignamini, A.; Borsa, F.; Claudi, R. U.; Covino, E.; Desidera, S.; Esposito, M.; Gratton, R.; González Hernández, J. I.; Lanza, A. F.; Maggio, A.; Molinari, E.; Pagano, I.; Perger, M.; Pillitteri, I.; Piotto, G.; Poretti, E.; Prisinzano, L.; Rebolo, R.; Ribas, I.; Shkolnik, E.; et al. Stellar parameters of early-M dwarfs from ratios of spectral features at optical wavelengths. Astronomy and Astrophysics. 2015, 577: A132. Bibcode:2015A&A...577A.132M. S2CID 53582613. arXiv:1503.03010
. doi:10.1051/0004-6361/201525797.
- ^ Lindgren, Sara; Heiter, Ulrike. Metallicity determination of M dwarfs. Expanded parameter range in metallicity and effective temperature. Astronomy and Astrophysics. 2017, 604: A97. Bibcode:2017A&A...604A..97L. S2CID 119216828. arXiv:1705.08785
. doi:10.1051/0004-6361/201730715.
- ^ Houdebine, E. R. Observation and modelling of main-sequence star chromospheres - XIV. Rotation of dM1 stars. Monthly Notices of the Royal Astronomical Society. 2010, 407 (3): 1657–1673. Bibcode:2010MNRAS.407.1657H. doi:10.1111/j.1365-2966.2010.16827.x
.
- ^ Gliese, W.; Jahreiß, H. Gl 908. Preliminary Version of the Third Catalogue of Nearby Stars. 1991 [2023-03-21]. (原始内容存档于2016-03-04).
- ^ Luyten, Willem Jacob. LHS 550. LHS Catalogue, 2nd Edition. 1979 [2023-03-21]. (原始内容存档于2020-09-25).
- ^ Van Altena W. F.; Lee J. T.; Hoffleit E. D. GCTP 5763. The General Catalogue of Trigonometric Stellar Parallaxes Fourth. 1995 [2023-03-21]. (原始内容存档于2016-03-04).
- ^ Perryman; et al. HIP 117473. The Hipparcos and Tycho Catalogues. 1997 [2023-03-21]. (原始内容存档于2016-03-04).
- ^ Weis, Edward W. Long Term Variability in Dwarf M Stars. The Astronomical Journal. 1994, 107: 1135. Bibcode:1994AJ....107.1135W. doi:10.1086/116925.
- ^ Kazarovets, E. V.; Samus, N. N. The 73rd Name-List of Variable Stars. Information Bulletin on Variable Stars. 1997, 4471: 1. Bibcode:1997IBVS.4471....1K.
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