Star in the constellation Vela
GX Velorum is a solitary[ 12] variable star [ 3] in the southern constellation of Vela . It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude that fluctuates around 4.99.[ 2] Based upon parallax measurements, it is located approximately 4,200 light years distant from the Sun, and is drifting further away with a radial velocity of +28 km/s.[ 6] It may be a member of the Vela OB1 association of co-moving stars.[ 7]
A light curve for GX Velorum, plotted from Hipparcos data[ 13]
This object is a massive blue supergiant with a stellar classification of B5 Ia.[ 4] It is suspected to be an Alpha Cygni-type pulsating variable and ranges in brightness from 4.97 down to 5.04 magnitude.[ 3] It is losing mass at the rate of (0.40± 0.02)× 10−6 M ☉ yr−1 ,[ 9] or one solar mass every 2.5 million years. The star is 8.3[ 10] million years old with 35 times the mass of the Sun .[ 8] It has expanded to around 61[ 9] times the Sun's radius and is radiating 214,000[ 9] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 15,000 K.[ 9]
References
^ a b c d e Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters . 38 (5): 331. arXiv :1108.4971 . Bibcode :2012AstL...38..331A . doi :10.1134/S1063773712050015 . S2CID 119257644 .
^ a b c d Samus', N. N; et al. (2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports . 61 (1): 80. Bibcode :2017ARep...61...80S . doi :10.1134/S1063772917010085 . S2CID 125853869 .
^ a b Houk, Nancy (1978). Michigan catalogue of two-dimensional spectral types for the HD stars . Vol. 2. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode :1978mcts.book.....H .
^ a b Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues . 2237 . Bibcode :2002yCat.2237....0D .
^ a b Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters . 32 (11): 759–771. arXiv :1606.08053 . Bibcode :2006AstL...32..759G . doi :10.1134/S1063773706110065 . S2CID 119231169 .
^ a b Reed, B. Cameron (2000). "Vela OB1: Probable New Members and Hertzsprung-Russell Diagram" . The Astronomical Journal . 119 (4): 1855–1859. Bibcode :2000AJ....119.1855R . doi :10.1086/301313 .
^ a b Fraser, M.; et al. (2010). "Atmospheric parameters and rotational velocities for a sample of Galactic B-type supergiants" . Monthly Notices of the Royal Astronomical Society . 404 (3): 1306. arXiv :1001.3337 . Bibcode :2010MNRAS.404.1306F . doi :10.1111/j.1365-2966.2010.16392.x . S2CID 118674151 .
^ a b c d e f g h Haucke, M.; et al. (June 2018), "Wind properties of variable B supergiants. Evidence of pulsations connected with mass-loss episodes", Astronomy & Astrophysics , 614 : 28, arXiv :1902.01341 , Bibcode :2018A&A...614A..91H , doi :10.1051/0004-6361/201731678 , S2CID 126150688 , A91
^ a b Tetzlaff, N.; et al. (2011). "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun" . Monthly Notices of the Royal Astronomical Society . 410 (1): 190–200. arXiv :1007.4883 . Bibcode :2011MNRAS.410..190T . doi :10.1111/j.1365-2966.2010.17434.x . S2CID 118629873 .
^ "GX Vel" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-08-16 .
^ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869–879. arXiv :0806.2878 . Bibcode :2008MNRAS.389..869E . doi :10.1111/j.1365-2966.2008.13596.x . S2CID 14878976 .
^ "Hipparcos Tools Interactive Data Access" . Hipparcos . ESA. Retrieved 8 December 2021 .