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宗正增二

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宗正增二(蛇夫座σ)
標示宗正增二位置(紅圈)的星圖。
觀測資料
曆元 J2000
星座 蛇夫座
星官 宗正天市垣
赤經 17h 26m 30.8806s[1]
赤緯 +04° 08′ 25.2876″[1]
視星等(V) 4.31[2] (4.25 - 4.51[3])
特性
光谱分类K2 III[4]
U−B 色指数+1.57[2]
B−V 色指数+1.51[2]
变星类型疑似[3]
天体测定
徑向速度 (Rv)−27.81[5] km/s
自行 (μ) 赤经:+1.459[6] mas/yr
赤纬:+6.760[6] mas/yr
视差 (π)3.7578 ± 0.1559[6] mas
距离870 ± 40 ly
(270 ± 10 pc)
绝对星等 (MV)−2.85[7]
詳細資料
質量5–9[8] M
半徑100±30[8] R
表面重力 (log g)1.3±0.5[8]
亮度2630±894[8] L
溫度4,129±566[8] K
金属量 [Fe/H]−0.07[9] dex
自轉速度 (v sin i)4.2[10] km/s
其他命名
σ Oph、​49 Ophiuchi、​NSV 8664、​BD+04°3422、​FK5 1459、​GC 23621、​HD 157999、​HIP 85355、​HR 6498、​SAO 122387、​2MASS J17263087+0408252
參考資料庫
SIMBAD资料

宗正增二蛇夫座σ),來自「σ Ophiuchi」的拉丁化,是在天球赤道星座蛇夫座的一顆單獨的巨大橘色恆星[11]。它的視星等為4.31等[2],其亮度足以用肉眼看見微弱的光點。從地球上看,每年3.62mas視差偏移,提供的距離估計大約900光年。它正以-28公里/秒的徑向速度靠近太陽[5]

這是一顆K型恆星,已經演化巨星,其恒星分類為K2 III[4]。維特科夫斯基(Wittkowski)等人(2017)認為它的光度為II-III,表明它位於巨星和超巨星之間的過渡區[8]。它的質量大約是太陽的5到9倍,半徑是太陽的100倍。這顆恆星的在4,130 K的有效溫度下,從其漲大的光球發出的輻射是太陽的2,600倍[8]

參考文獻

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  1. ^ 1.0 1.1 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 Ducati, J. R. VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system. CDS/ADC Collection of Electronic Catalogues. 2002, 2237. Bibcode:2002yCat.2237....0D. 
  3. ^ 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. Bibcode:2009yCat....102025S. 
  4. ^ 4.0 4.1 Houk, N.; Swift, C. Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5. Michigan Spectral Survey. 1999, 05: 0. Bibcode:1999MSS...C05....0H. 
  5. ^ 5.0 5.1 Famaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Astronomy & Astrophysics. 2005, 430: 165–186. Bibcode:2005A&A...430..165F. S2CID 17804304. arXiv:astro-ph/0409579可免费查阅. doi:10.1051/0004-6361:20041272. 
  6. ^ 6.0 6.1 6.2 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可免费查阅. doi:10.1051/0004-6361/202039657可免费查阅.  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.
  7. ^ 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.  Vizier catalog entry
  8. ^ 8.0 8.1 8.2 8.3 8.4 8.5 8.6 Wittkowski, M.; et al, VLTI/AMBER spectro-interferometry of the late-type supergiants V766 Cen (=HR 5171 A), σ Oph, BM Sco, and HD 206859, Astronomy & Astrophysics, January 2017, 597: 16, Bibcode:2017A&A...597A...9W, S2CID 55679854, arXiv:1610.01927可免费查阅, doi:10.1051/0004-6361/201629349, A9. 
  9. ^ Reffert, Sabine; Bergmann, Christoph; Quirrenbach, Andreas; Trifonov, Trifon; Künstler, Andreas. Precise radial velocities of giant stars. Astronomy & Astrophysics. 2015, 574: A116. Bibcode:2015A&A...574A.116R. S2CID 59334290. arXiv:1412.4634可免费查阅. doi:10.1051/0004-6361/201322360. hdl:10722/215277.  Vizier catalog entry
  10. ^ De Medeiros, J. R.; Mayor, M. A catalog of rotational and radial velocities for evolved stars. Astronomy and Astrophysics Supplement Series. 1999, 139 (3): 433. Bibcode:1999A&AS..139..433D. arXiv:astro-ph/0608248可免费查阅. doi:10.1051/aas:1999401.  Vizier catalog entry
  11. ^ 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.