水位二

水位二(小犬座11)
觀測資料
曆元 J2000.0 (ICRS)
星座 小犬座
星官 水位鬼宿
赤經 07h 46m 16.20081s[1]
赤緯 +10° 46′ 05.7055″[1]
視星等(V) 5.25[2]
特性
光谱分类A1Vnn[3]
B−V 色指数0.018±0.008[2]
天体测定
徑向速度 (Rv)+28.0±4.2[4] km/s
自行 (μ) 赤经:−29.902[1] mas/yr
赤纬:−25.275[1] mas/yr
视差 (π)10.4262 ± 0.2007[1] mas
距离313 ± 6 ly
(96 ± 2 pc)
绝对星等 (MV)0.42[2]
詳細資料
質量2.23[5] M
半徑2.5[6] R
表面重力 (log g)3.60[5]
亮度65.26[2] L
溫度9,972±339[5] K
年齡149[5] Myr
其他命名
11 CMi、​NSV 3724、​BD+11°1670、​FK5 1201、​GC 10463、​HD 62832、​HIP 37921、​HR 3008、​SAO 97224[7]
參考資料庫
SIMBAD资料

水位二也稱為小犬座11是在赤道星座小犬座 [7]的一顆恆星[8],距離太陽約313光年[1]。它是一顆肉眼可見的微弱白色恒星,視星等為+5.25[2]。它正以相對於日心+28公里/秒的徑向速度遠離地球[4],大約235萬年前的距離在157光年以內[2]

這是一顆A型主序星,其恆星分類為A1Vnn[3],其中的符號「n」表示由於快速旋轉而導致的(非常)「模糊」。然而,Gray和Garrison(1987)發現了一個A0.5Ivnn的分類[9],這將與一顆演化次巨星相匹配。這是一顆未知類型的可疑變星[10]。它的年齡為1億4900萬年[5],質量是2.23倍太陽質量[5],半徑是2.5倍太陽半徑[6]。它以9,972K的有效溫度[5]光球層輻射65倍的太陽光度[2]

參考資料

  1. ^ 1.0 1.1 1.2 1.3 1.4 1.5 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可免费查阅. 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
  2. ^ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Anderson, E.; Francis, Ch., XHIP: An extended hipparcos compilation, Astronomy Letters, 2012, 38 (5): 331, Bibcode:2012AstL...38..331A, S2CID 119257644, arXiv:1108.4971可免费查阅, doi:10.1134/S1063773712050015. 
  3. ^ 3.0 3.1 Cowley, A.; et al, A study of the bright A stars. I. A catalogue of spectral classifications, Astronomical Journal, April 1969, 74: 375–406, Bibcode:1969AJ.....74..375C, doi:10.1086/110819. 
  4. ^ 4.0 4.1 Gontcharov, G. A., Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system, Astronomy Letters, November 2006, 32 (11): 759–771, Bibcode:2006AstL...32..759G, S2CID 119231169, arXiv:1606.08053可免费查阅, doi:10.1134/S1063773706110065. 
  5. ^ 5.0 5.1 5.2 5.3 5.4 5.5 5.6 David, Trevor J.; Hillenbrand, Lynne A., The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets, The Astrophysical Journal, 2015, 804 (2): 146, Bibcode:2015ApJ...804..146D, S2CID 33401607, arXiv:1501.03154可免费查阅, doi:10.1088/0004-637X/804/2/146. 
  6. ^ 6.0 6.1 Pasinetti Fracassini, L. E.; et al, Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS), Astronomy and Astrophysics Third, February 2001, 367 (2): 521–524, Bibcode:2001A&A...367..521P, S2CID 425754, arXiv:astro-ph/0012289可免费查阅, doi:10.1051/0004-6361:20000451. 
  7. ^ 7.0 7.1 11 CMi. SIMBAD. 斯特拉斯堡天文資料中心. 
  8. ^ Eggleton, P. P.; Tokovinin, A. A., A catalogue of multiplicity among bright stellar systems, Monthly Notices of the Royal Astronomical Society, September 2008, 389 (2): 869–879, Bibcode:2008MNRAS.389..869E, S2CID 14878976, arXiv:0806.2878可免费查阅, doi:10.1111/j.1365-2966.2008.13596.x可免费查阅. 
  9. ^ Gray, R. O.; Garrison, R. F., The Early A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation, Astrophysical Journal Supplement, December 1987, 65: 581, Bibcode:1987ApJS...65..581G, doi:10.1086/191237可免费查阅. 
  10. ^ Samus, N. N.; et al, General Catalogue of Variable Stars, Astronomy Reports, 5.1, 2017, 61 (1): 80–88, Bibcode:2017ARep...61...80S, S2CID 125853869, doi:10.1134/S1063772917010085. 

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