HD 211575

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HD 211575
File:HD 211575.png
HD 211575 的周边地区
观测资料
历元 J2000
星座 宝瓶座[1]
星官
赤经 22h 18m 04.2722s[2]
赤纬 −00° 14′ 15.557″[2]
视星等(V) 6.40[3]
特性
光谱分类F3 V[4]
B−V 色指数0.441±0.003[1]
天体测定
径向速度 (Rv)+14.8±0.5[5] km/s
自行 (μ) 赤经:−41.997[2] mas/yr
赤纬:+54.407[2] mas/yr
视差 (π)24.13 ± 0.29[6] mas
距离135 ± 2 ly
(41.4 ± 0.5 pc)
绝对星等 (MV)3.31[3]
详细资料
质量1.27[7] M
表面重力 (log g)4.15[3]
亮度4.30[1] L
温度6,574±224[7] K
金属量 [Fe/H]+0.11±0.11[5] dex
自转速度 (v sin i)19.0[3] km/s
年龄150[5] Myr
其他命名
BD−00°4333、​HD 203222、​HIP 110091、​HR 8507、​SAO 146004[8]
参考数据库
SIMBAD资料

HD 211575位于星座 宝瓶座,介于坟墓二(宝瓶座γ)、坟墓四(宝瓶座π)和危宿一(宝瓶座α)之间。它是大熊座移动星群的冠状体的成员[9]

参考文献[编辑]

  1. ^ 1.0 1.1 1.2 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. 
  2. ^ 2.0 2.1 2.2 2.3 Brown, A. G. A.; et al, Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties, Astronomy and Astrophysics, 2016, 595, A2, Bibcode:2016A&A...595A...2G, S2CID 1828208, arXiv:1609.04172可免费查阅, doi:10.1051/0004-6361/201629512. 
  3. ^ 3.0 3.1 3.2 3.3 Paunzen, E.; et al, Investigating the possible connection between λ Bootis stars and intermediate Population II type stars, Astronomy & Astrophysics, July 2014, 567: 8, Bibcode:2014A&A...567A..67P, S2CID 56332289, arXiv:1406.3936可免费查阅, doi:10.1051/0004-6361/201423817, A67. 
  4. ^ Houk, N.; Swift, C., Michigan catalogue of two-dimensional spectral types for the HD Stars, Michigan Spectral Survey, 1999, 5, Bibcode:1999MSS...C05....0H. 
  5. ^ 5.0 5.1 5.2 Casagrande, L.; et al, New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey, Astronomy & Astrophysics, 2011, 530 (A138): 21, Bibcode:2011A&A...530A.138C, S2CID 56118016, arXiv:1103.4651可免费查阅, doi:10.1051/0004-6361/201016276. 
  6. ^ van Leeuwen, F., Validation of the new Hipparcos reduction, Astronomy and Astrophysics, 2007, 474 (2): 653–664, Bibcode:2007A&A...474..653V, S2CID 18759600, arXiv:0708.1752可免费查阅, doi:10.1051/0004-6361:20078357. 
  7. ^ 7.0 7.1 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. 
  8. ^ HD 211575. SIMBAD. 斯特拉斯堡天文资料中心. 
  9. ^ Chupina, N. V.; et al, Kinematic structure of the corona of the Ursa Major flow found using proper motions and radial velocities of single stars, Astronomy and Astrophysics, June 2006, 451 (3): 909−916, Bibcode:2006A&A...451..909C, doi:10.1051/0004-6361:20054009可免费查阅.