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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.
With an apparent magnitude of 1.8, its brightest star is the hot blue multiple star Gamma Velorum, one component of which is the closest and brightest Wolf-Rayet star in the sky. Delta and Kappa Velorum, together with Epsilon and Iota Carinae, form the asterism known as the False Cross. 1.95-magnitude Delta is actually a triple or quintuple ...
Gamma Velorum has the traditional name Al Suhail al Muhlif, [specify] also known as Regor. Zeta Puppis, in the constellation of Puppis, is traditionally known as Suhail Hadar (سهيل هدار). In addition to these, the star Canopus (α Carinae), the second-brightest star in the night sky, is called in Arabic: سهيل, romanized: suhayl or ...
Bayer assigned a lowercase Greek letter (alpha (α), beta (β), gamma (γ), etc.) or a Latin letter (A, b, c, etc.) to each star he catalogued, combined with the Latin name of the star's parent constellation in genitive (possessive) form. The constellation name is frequently abbreviated to a standard three-letter form.
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Lambda Velorum (λ Velorum, abbreviated Lambda Vel, λ Vel), officially named Suhail / ˈ s uː h eɪ l /, [11] is a star in the southern constellation of Vela.With a mean apparent visual magnitude of 2.21, [2] this is the third-brightest star in the constellation and one of the brighter stars in the sky.
Vela X-1 is a pulsing, eclipsing high-mass X-ray binary (HMXB) system, associated with the Uhuru source 4U 0900-40 and the supergiant star HD 77581. The X-ray emission of the neutron star is caused by the capture and accretion of matter from the stellar wind of the supergiant companion. Vela X-1 is the prototypical detached HMXB.
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