大犬座ι

天狼增五Iota Canis Majoris)的拉丁化源自ι Canis Majoris,孤獨的[12]位在南天星座大犬座,是一顆超巨星變星。它的視星等在+4.36和+4.40之間變化著[3]。根據視差的測量,這顆恆星與地球相距約3,100光年。它正以+41.2Km/s的徑向速度遠離而去[7]

天狼增五(大犬座ι)
天狼增五在大犬座的位置(紅圈)。
觀測資料
曆元 J2000
星座 大犬座
星官 天狼井宿
赤經 06h 56m 08.22413s[1]
赤緯 −17° 03′ 15.2675″[1]
視星等(V) 4.40[2] (4.36 - 4.40[3])
特性
光谱分类B3Ib[4],或B3Ib/II[5]
U−B 色指数−0.74[6]
B−V 色指数−0.07[6]
变星类型仙王座β型?[2]
天体测定
徑向速度 (Rv)+41.20[7] km/s
自行 (μ) 赤经:−3.56 ± 0.17[1] mas/yr
赤纬:+2.42 ±0.20[1] mas/yr
视差 (π)1.04 ± 0.20[1] mas
距离approx. 3,100 ly
(approx. 1,000 pc)
绝对星等 (MV)−5.51[8]
詳細資料
質量12.5[9] M
半徑25.9[8] R
表面重力 (log g)2.60[10]
亮度47,000[8] L
溫度17,000[10] K
金属量 [Fe/H]−0.17[11] dex
自轉速度 (v sin i)27±4[10] km/s
年齡14.8[9] Myr
其他命名
ι CMa、​20 Canis Majoris、​BD−16°1661、​FK5 2536、​GC 9107、​HD 51309、​HIP 33347、​HR 2596、​SAO 152126
參考資料庫
SIMBAD资料

天狼增五是一顆大質量的藍白色B型超巨星,光譜類型為B3Ib[4]。它被歸類為仙王座β型變星[3],但超巨星光譜類型和一個多月的期意味著它不再被認為是這種類型的[2]。這顆恆星的年齡為1,480萬,並正以27Km/s投影旋轉速度自轉[10]。它的質量是太陽的12.5倍[9],半徑是太陽的25.9倍[8]。天狼增五的光度是太陽的47,000倍[8]光球層有效溫度是17,000K[10]

這顆恆星在與星際物質的相互作用中顯示出弓形激波特徵,但這種星雲與恆星在銀河系中的運動不一致[13]

參考資料

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  2. ^ 2.0 2.1 2.2 Stankov, Anamarija; Handler, Gerald. Catalog of Galactic β Cephei Stars. The Astrophysical Journal Supplement Series. 2005, 158 (2): 193–216. Bibcode:2005ApJS..158..193S. ISSN 0067-0049. S2CID 119526948. arXiv:astro-ph/0506495 . doi:10.1086/429408. 
  3. ^ 3.0 3.1 3.2 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: 02025. Bibcode:2009yCat....102025S. 
  4. ^ 4.0 4.1 Prinja, R. K.; Massa, D. L. Signature of wide-spread clumping in B supergiant winds. Astronomy and Astrophysics. 2010, 521: L55. Bibcode:2010A&A...521L..55P. ISSN 0004-6361. S2CID 59151633. arXiv:1007.2744 . doi:10.1051/0004-6361/201015252. 
  5. ^ Houk, Nancy; Smith-Moore, M. Michigan catalogue of two-dimensional spectral types for the HD stars 4. Ann Arbor: Dept. of Astronomy, University of Michigan. 1978. Bibcode:1988mcts.book.....H. 
  6. ^ 6.0 6.1 Mermilliod, J.-C. Compilation of Eggen's UBV data, transformed to UBV (unpublished). Catalogue of Eggen's UBV Data. 1986. Bibcode:1986EgUBV........0M. 
  7. ^ 7.0 7.1 Gontcharov, G. A. Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system. Astronomy Letters. 2006, 32 (11): 759–771. Bibcode:2006AstL...32..759G. ISSN 1063-7737. S2CID 119231169. arXiv:1606.08053 . doi:10.1134/S1063773706110065. 
  8. ^ 8.0 8.1 8.2 8.3 8.4 Balona, L. A.; Engelbrecht, C. A. Photometry and frequency analysis of line profile variables. Monthly Notices of the Royal Astronomical Society. 1985, 214 (4): 559. Bibcode:1985MNRAS.214..559B. doi:10.1093/mnras/214.4.559 . 
  9. ^ 9.0 9.1 9.2 Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun. Monthly Notices of the Royal Astronomical Society. 2011, 410: 190–200. Bibcode:2011MNRAS.410..190T. S2CID 118629873. arXiv:1007.4883 . doi:10.1111/j.1365-2966.2010.17434.x. 
  10. ^ 10.0 10.1 10.2 10.3 10.4 Lefever, K.; Puls, J.; Morel, T.; Aerts, C.; Decin, L.; Briquet, M. Spectroscopic determination of the fundamental parameters of 66 B-type stars in the field-of-view of the CoRoT satellite. Astronomy and Astrophysics. 2010, 515: A74. Bibcode:2010A&A...515A..74L. S2CID 54028925. arXiv:0910.2851 . doi:10.1051/0004-6361/200911956. 
  11. ^ Gies, Douglas R.; Lambert, David L. Carbon, nitrogen, and oxygen abundances in early B-type stars. Astrophysical Journal. 1992, 387: 673. Bibcode:1992ApJ...387..673G. doi:10.1086/171116. 
  12. ^ 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 . doi:10.1111/j.1365-2966.2008.13596.x. 
  13. ^ Bodensteiner, J.; Baade, D.; Greiner, J.; Langer, N. Infrared nebulae around bright massive stars as indicators for binary interactions. Astronomy & Astrophysics. October 2018, 618: 13. Bibcode:2018A&A...618A.110B. S2CID 118972162. arXiv:1806.01294 . doi:10.1051/0004-6361/201832722. A110.