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天鹅座ω1

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天鹅座ω1

天鹅座V2014的光变曲线
根据“TESS”的数据绘制[1]
观测资料
历元 J2000.0
星座 天鹅座
星官 天津女宿
赤经 20h 30m 03.54116s[2]
赤纬 +48° 57′ 05.6446″[2]
视星等(V) +4.93 - 4.96[3]
特性
光谱分类B2.5 IV[4]
U−B 色指数−0.68[5]
B−V 色指数−0.09[5]
变星类型仙王座β[6] 波江座λ[3]
天体测定
径向速度 (Rv)−21.9±2.0[7] km/s
自行 (μ) 赤经:+10.883[8] mas/yr
赤纬:+7.057[8] mas/yr
视差 (π)2.5878 ± 0.1637[8] mas
距离1,260 ± 80 ly
(390 ± 20 pc)
绝对星等 (MV)−2.65[9]
详细资料
质量8.1±0.2[4] M
半径13.825[10] R
表面重力 (log g)2.312[10]
亮度1,549[11] L
温度16,982[11] K
金属量 [Fe/H]0.0[9] dex
自转速度 (v sin i)145[12] km/s
年龄33.2±4.5[4] Myr
其他命名
ω1 Cyg45 Cygni、BD+48°3142、FK5 3641、HD 195556、HIP 101138、HR 7844、SAO 49712、V2014 Cygni[13]
参考数据库
SIMBAD资料

天鹅座ω1,来自拉丁化ω1 Cygni,是独立的拜耳名称[14],它是在北天星座天鹅座的一颗恒星;中文传统名称是天津增卅五。它的视星等为4.94[5],以肉眼即可看见。基于2.59mas的周年视差偏移[8],估计它与太阳的距离大约为1,260 光年。相对于它的邻居,这颗恒星的本动速度25.7±2.2 km/s[7]

这是一颗有点演化B型次巨星恒星分类为B2.5 IV[4]。Telting及其同事在2006年发表的一项高分辨率光谱学研究中指出,在其光谱中发现了规则的脉动,因此他们对此高度自信,它是一颗仙王座β型变星[6]。它的亮度每1.137天不规则地变化0.034星等[15]

相关条目

参考资料

  1. ^ MAST: Barbara A. Mikulski Archive for Space Telescopes. Space Telescope Science Institute. [27 November 2022]. (原始内容存档于2023-03-27). 
  2. ^ 2.0 2.1 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. 
  3. ^ 3.0 3.1 V2014 Cygni, International Variable Star Index, [2020-09-02], (原始内容存档于2023-08-12) 
  4. ^ 4.0 4.1 4.2 4.3 Tetzlaff, N.; et al, A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun, Monthly Notices of the Royal Astronomical Society, 2011, 410 (1): 190–200, Bibcode:2011MNRAS.410..190T, S2CID 118629873, arXiv:1007.4883可免费查阅, doi:10.1111/j.1365-2966.2010.17434.x. 
  5. ^ 5.0 5.1 5.2 Mermilliod, J.-C., Compilation of Eggen's UBV data, transformed to UBV (unpublished), Catalogue of Eggen's UBV Data (SIMBAD), 1986, Bibcode:1986EgUBV........0M. 
  6. ^ 6.0 6.1 Telting, J. H.; et al, A high-resolution spectroscopy survey of β Cephei pulsations in bright stars, Astronomy and Astrophysics, June 2006, 452 (3): 945–953, Bibcode:2006A&A...452..945T, doi:10.1051/0004-6361:20054730可免费查阅. 
  7. ^ 7.0 7.1 Bobylev, V. V.; Bajkova, A. T., Galactic kinematics from a sample of young massive stars, Astronomy Letters, August 2013, 39 (8): 532–549, Bibcode:2013AstL...39..532B, S2CID 118568203, arXiv:1307.1677可免费查阅, doi:10.1134/S106377371308001X. 
  8. ^ 8.0 8.1 8.2 8.3 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
  9. ^ 9.0 9.1 Gontcharov, G. A., Dependence of kinematics on the age of stars in the solar neighborhood, Astronomy Letters, 2012, 38 (12): 771–782, Bibcode:2012AstL...38..771G, S2CID 118345778, arXiv:1606.08814可免费查阅, doi:10.1134/S1063773712120031. 
  10. ^ 10.0 10.1 McDonald, I.; Zijlstra, A. A.; Watson, R. A., Fundamental parameters and infrared excesses of Tycho–Gaia stars, Monthly Notices of the Royal Astronomical Society, 2017, 471 (1): 770–791, Bibcode:2017MNRAS.471..770M, S2CID 73594365, arXiv:1706.02208可免费查阅, doi:10.1093/mnras/stx1433. 
  11. ^ 11.0 11.1 Simón-Díaz, S.; Godart, M.; Castro, N.; Herrero, A.; Aerts, C.; Puls, J.; Telting, J.; Grassitelli, L., The IACOB project . III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars, Astronomy and Astrophysics, 2017, 597: A22, Bibcode:2017A&A...597A..22S, S2CID 3478126, arXiv:1608.05508可免费查阅, doi:10.1051/0004-6361/201628541. 
  12. ^ Abt, Helmut A.; Levato, Hugo; Grosso, Monica, Rotational Velocities of B Stars, The Astrophysical Journal, July 2002, 573 (1): 359–365, Bibcode:2002ApJ...573..359A, doi:10.1086/340590可免费查阅. 
  13. ^ * ome01 Cyg -- Pulsating variable Star. SIMBAD. 斯特拉斯堡天文资料中心. 
  14. ^ 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. 
  15. ^ Lefèvre, L.; et al, A systematic study of variability among OB-stars based on HIPPARCOS photometry, Astronomy and Astrophysics, 2009, 507 (2): 1141, Bibcode:2009A&A...507.1141L, doi:10.1051/0004-6361/200912304可免费查阅.