Star system in the constellation Vela
γ2 Velorum
Location of γ Velorum (circled)
Observation dataEpoch J2000 Equinox J2000
Constellation
Vela
Right ascension
08h 09m 31.95013s [ 1]
Declination
–47° 20′ 11.7108″[ 1]
Apparent magnitude (V)
1.83[ 2] (1.81–1.87[ 3] )
Characteristics
Spectral type
WC8 + O7.5III[ 4]
U−B color index
−0.94[ 2]
B−V color index
−0.25[ 2]
Variable type
Wolf–Rayet [ 3]
Astrometry Radial velocity (Rv )+12 ± 1[ 5] km/s Proper motion (μ) RA: –6.07[ 1] mas /yr Dec.: +10.43[ 1] mas /yr Parallax (π)2.92 ± 0.30 mas [ 1] Distance 1096+26 −23 ly ( 336+8 −7 [ 6] pc )Absolute magnitude (MV )−4.6 + −6.0 [ 6]
Orbit [ 7] Primary O Companion WR Period (P)78.53 ± 0.01 days Semi-major axis (a)1.2[ 8] AU Eccentricity (e)0.326 ± 0.01 Inclination (i)65 ± 8° Periastron epoch (T)2,450,120.5 ± 2 Argument of periastron (ω) (secondary)248 ± 4° Semi-amplitude (K1 ) (primary)38.4 ± 2 km/s Semi-amplitude (K2 ) (secondary)122 ± 2 km/s
Details WR Mass 9.0 ± 0.6 [ 8] M ☉ Radius 1.9[ 6] R ☉ Luminosity (bolometric) 204,000[ 6] L ☉ Luminosity (visual, LV ) 5,900[ 6] L ☉ Temperature 90,000[ 6] K Age 5[ 6] Myr O Mass 28.5 ± 1.1[ 8] M ☉ Radius 16.2[ 6] R ☉ Luminosity (bolometric) 363,000[ 6] L ☉ Luminosity (visual, LV ) 21,500[ 6] L ☉ Temperature 35,100[ 6] K Age 5[ 6] Myr
Other designations Regor, Suhail Al-Muhlif,
CD −46°3847,
FK5 309,
HD 68273,
HIP 39953,
HR 3207,
SAO 219504,
WR 11
Database references SIMBAD data
Gamma Velorum is a quadruple star system in the constellation Vela . This name is the Bayer designation for the star, which is Latinised from γ Velorum and abbreviated γ Vel . At a combined magnitude of +1.72, it is one of the brightest stars in the night sky , and contains by far the closest and brightest Wolf–Rayet star . It has the traditional name Suhail al Muhlif and the modern name Regor ,[ 13] but neither is approved by the International Astronomical Union , making it the brightest star by apparent magnitude without an IAU approved name.
The γ Velorum system includes a pair of stars separated by 41″, each of which is also a spectroscopic binary system. γ2 Velorum, the brighter of the visible pair, contains the Wolf–Rayet star and a blue supergiant , while γ1 Velorum contains a blue giant and an unseen companion.
^ a b c d e van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 474 (2): 653–664, arXiv :0708.1752 , Bibcode :2007A&A...474..653V , doi :10.1051/0004-6361:20078357 , S2CID 18759600
^ a b c 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 : 0. Bibcode :2002yCat.2237....0D .
^ a b Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007–2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S . 1 : 02025. Bibcode :2009yCat....102025S .
^ Roche, P. F.; Colling, M. D.; Barlow, M. J. (2012). "The outer wind of γ Velorum" . Monthly Notices of the Royal Astronomical Society . 427 (1): 581. arXiv :1208.6016 . Bibcode :2012MNRAS.427..581R . doi :10.1111/j.1365-2966.2012.22005.x . S2CID 119234167 .
^ Niemela, V. S.; Sahade, J. (1980). "The orbital elements of Gamma 2 Velorum". The Astrophysical Journal . 238 : 244. Bibcode :1980ApJ...238..244N . doi :10.1086/157981 . ISSN 0004-637X .
^ a b c d e f g h i j k l Crowther, Paul A.; Barlow, M. J.; Royer, P.; Hillier, D. J.; Bestenlehner, J. M.; Morris, P. W.; Wesson, R. (2024-01-01). "Oxygen abundance of γ Vel from [O III] 88μm Herschel/PACS spectroscopy" . Monthly Notices of the Royal Astronomical Society . 528 (2): 2026. arXiv :2310.15170 . Bibcode :2024MNRAS.528.2026C . doi :10.1093/mnras/stae145 . ISSN 0035-8711 .
^ Schmutz, W.; Schweickhardt, J.; Stahl, O.; Wolf, B.; Dumm, T.; Gang, Th.; Jankovics, I.; Kaufer, A.; Lehmann, H.; Mandel, H.; Peitz, J.; Rivinius, Th. (1997). "The orbital motion of gamma^2 Velorum". Astronomy and Astrophysics . 328 : 219. Bibcode :1997A&A...328..219S .
^ a b c North, J. R.; Tuthill, P. G.; Tango, W. J.; Davis, J. (2007). "Γ2 Velorum: Orbital solution and fundamental parameter determination with SUSI" . Monthly Notices of the Royal Astronomical Society . 377 (1): 415–424. arXiv :astro-ph/0702375 . Bibcode :2007MNRAS.377..415N . doi :10.1111/j.1365-2966.2007.11608.x . S2CID 16425744 .
^ a b Hog, E.; Kuzmin, A.; Bastian, U.; Fabricius, C.; Kuimov, K.; Lindegren, L.; Makarov, V. V.; Roeser, S. (1998). "The TYCHO Reference Catalogue". Astronomy and Astrophysics . 335 : L65. Bibcode :1998A&A...335L..65H .
^ a b c d Hernandez, C. A.; Sahade, J. (1980). "The Spectroscopic Binary GAMMA-1-VELORUM". Publications of the Astronomical Society of the Pacific . 92 : 819. Bibcode :1980PASP...92..819H . doi :10.1086/130756 . ISSN 0004-6280 . S2CID 120181128 .
^ a b c d Cite error: The named reference jeffries
was invoked but never defined (see the help page ).
^ a b Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics . 355 : L27. Bibcode :2000A&A...355L..27H . doi :10.1888/0333750888/2862 .
^ Kunitzsch, Paul; Smart, Tim (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, Massachusetts: Sky Pub. ISBN 978-1-931559-44-7 .