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  2. Gamma Velorum - Wikipedia

    en.wikipedia.org/wiki/Gamma_Velorum

    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.

  3. Vela (constellation) - Wikipedia

    en.wikipedia.org/wiki/Vela_(constellation)

    AH Velorum is a Cepheid variable located less than a degree to the northeast of Gamma. [19] A yellow-white supergiant of spectral type F7Ib-II, it pulsates between magnitudes 5.5 and 5.89 over 4.2 days. [20] Also lying close to Gamma, [21] V Velorum is a Cepheid of spectral type F6-F9II ranging from magnitude 7.2 to 7.9 over 4.4 days. [22]

  4. HD 77258 - Wikipedia

    en.wikipedia.org/wiki/HD_77258

    It has the Bayer designation w Velorum, while HD 77258 is the identifier from the Henry Draper Catalogue. The system is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.45. [2] It is located at a distance of approximately 218 light years from the Sun based on parallax. [1]

  5. List of stars in Vela - Wikipedia

    en.wikipedia.org/wiki/List_of_stars_in_Vela

    This is the list of notable stars in the constellation Vela, sorted by decreasing brightness.. This constellation's Bayer designations (Greek-letter star names) were given while it was still considered part of the constellation of Argo Navis.

  6. List of brightest natural objects in the sky - Wikipedia

    en.wikipedia.org/wiki/List_of_brightest_natural...

    Gamma Velorum: Double star 1.71 Alpha Gruis: Star 1.77 1.75 Alioth: Star 1.77 Alnitak: Triple star system 1.79 Alpha Persei: Star 1.79 Dubhe: Binary star system 1.84 Delta Canis Majoris: Star 1.85 Epsilon Sagittarii: Binary star system 1.85 Theta Scorpii: Binary star system 1.86 Alkaid: Star 1.86 Epsilon Carinae: Binary star system 1.87 [16 ...

  7. Wolf–Rayet star - Wikipedia

    en.wikipedia.org/wiki/Wolf–Rayet_star

    WR 136, a WN6 star where the atmosphere shed during the red supergiant phase has been shocked by the hot, fast WR winds to form a visible bubble nebula. In 1867, using the 40 cm Foucault telescope at the Paris Observatory, astronomers Charles Wolf and Georges Rayet [1] discovered three stars in the constellation Cygnus (HD 191765, HD 192103 and HD 192641, now designated as WR 134, WR 135, and ...

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