船帆座AH是在船帆座的一颗黄白色调单星[11]。它的平均视星等为5.70等[2],这使得必须在良好的观测条件下,才能用裸眼隐约看到它。从它的周年视差 1.217 mas[1]估计,它的距离大约是2,700光年。它正以每秒 +26公里的日心径向速度朝向地球移动[7]

船帆座AH
观测资料
历元 J2000
星座 船帆座
星官
赤经 08h 11m 59.96702s[1]
赤纬 -46° 38′ 39.6561″[1]
视星等(V) 5.70[2] (5.50 – 5.89)[3]
特性
光谱分类F7 Ib-II[4]
U−B 色指数0.39[5]
B−V 色指数0.59[6]
R−I 色指数[5]
变星类型仙王座δ[3]
天体测定
径向速度 (Rv)+26.0±2.9[7] km/s
自行 (μ) 赤经:−4.405[1] mas/yr
赤纬:+6.768[1] mas/yr
视差 (π)1.2170 ± 0.0570[1] mas
距离2,700 ± 100 ly
(820 ± 40 pc)
绝对星等 (MV)−2.52[8]
详细资料
质量7.0±0.5[9] M
表面重力 (log g)1.66[6]
亮度929.98[8] L
温度6,102[6] K
金属量 [Fe/H]+0.09[6] dex
自转速度 (v sin i)10.0±0.5[10] km/s
年龄50.0±11.0[9] Myr
其他命名
CD−46° 3902、​HD 68808、​HIP 40155、​HR 3232、​SAO 219587[5]
参考资料库
SIMBAD资料
NASA凌日系外行星巡天卫星(TESS)纪录的经典造父变星船帆座AH的光变曲线

它是颗光谱类型为F7Ib-II的亮巨星/超巨星 [12],年龄大约5,000万年[9]投影转动速度为每秒10公里[10]。它的质量为7太阳质量[9],来自有效温度6,102K[6]光球亮度是太阳的930倍[8]

这颗经典造父变星[3]视星等范围从5.50至5.89等,周期超过4.227171天[12]。它的第一泛音脉动有6.04天的基本周期[2]

参考资料

编辑
  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 . 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 Evans, Nancy Remage; Bond, Howard E; Schaefer, Gail H; Mason, Brian D; Tingle, Evan; Karovska, Margarita; Pillitteri, Ignazio. Hubble Space Telescope Snapshot Survey for Resolved Companions of Galactic Cepheids. The Astronomical Journal. 2016, 151 (5): 129. Bibcode:2016AJ....151..129E. arXiv:1603.02224 . doi:10.3847/0004-6256/151/5/129. 
  3. ^ 3.0 3.1 3.2 Samus', N. N; Kazarovets, E. V; Durlevich, O. V; Kireeva, N. N; Pastukhova, E. N. General catalogue of variable stars: Version GCVS 5.1. Astronomy Reports. 2017, 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. 
  4. ^ Houk, Nancy. Michigan catalogue of two-dimensional spectral types for the HD stars. Ann Arbor : Dept. Of Astronomy (Ann Arbor). 1978, 2. Bibcode:1978mcts.book.....H. 
  5. ^ 5.0 5.1 5.2 HD 68808. SIMBAD. 斯特拉斯堡天文资料中心. 
  6. ^ 6.0 6.1 6.2 6.3 6.4 Luck, R. Earle. Parameters and Abundances in Luminous Stars. The Astronomical Journal. 2014, 147 (6): 137. Bibcode:2014AJ....147..137L. doi:10.1088/0004-6256/147/6/137 . 
  7. ^ 7.0 7.1 de Bruijne, J. H. J.; Eilers, A.-C. Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project. Astronomy & Astrophysics. October 2012, 546: 14. Bibcode:2012A&A...546A..61D. arXiv:1208.3048 . doi:10.1051/0004-6361/201219219. A61. 
  8. ^ 8.0 8.1 8.2 Anderson, E.; Francis, Ch. XHIP: An extended hipparcos compilation. Astronomy Letters. 2012, 38 (5): 331. Bibcode:2012AstL...38..331A. arXiv:1108.4971 . doi:10.1134/S1063773712050015. 
  9. ^ 9.0 9.1 9.2 9.3 Tetzlaff, N.; et al, A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun, Monthly Notices of the Royal Astronomical Society, January 2011, 410 (1): 190–200, Bibcode:2011MNRAS.410..190T, arXiv:1007.4883 , doi:10.1111/j.1365-2966.2010.17434.x 
  10. ^ 10.0 10.1 Ammler-von Eiff, M.; Reiners, A. New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?. Astronomy & Astrophysics. June 2012, 542: A116. Bibcode:2012A&A...542A.116A. arXiv:1204.2459 . doi:10.1051/0004-6361/201118724. 
  11. ^ Eggleton, P. P.; Tokovinin, A. A. A catalogue of multiplicity among bright stellar systems. Monthly Notices of the Royal Astronomical Society. 2008, 389 (2): 869. Bibcode:2008MNRAS.389..869E. arXiv:0806.2878 . doi:10.1111/j.1365-2966.2008.13596.x. 
  12. ^ 12.0 12.1 Watson, Christopher. AH Velorum. AAVSO Website. American Association of Variable Star Observers. 4 January 2010 [12 March 2014]. (原始内容存档于2020-08-10).