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  2. Epsilon Aurigae - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Aurigae

    Epsilon Aurigae (ε Aurigae, abbreviated Epsilon Aur, ε Aur) is a multiple star system in the northern constellation of Auriga, the charioteer.It is an unusual eclipsing binary system comprising an F0 supergiant (officially named Almaaz / æ l ˈ m ɑː z /, the traditional name for the system) and a companion which is generally accepted to be a huge dark disk orbiting an unknown object ...

  3. Capella - Wikipedia

    en.wikipedia.org/wiki/Capella

    With an average apparent magnitude of +0.08, Capella is the brightest object in the constellation Auriga, the sixth-brightest star in the night sky, the third-brightest in the northern celestial hemisphere (after Arcturus and Vega), and the fourth-brightest visible to the naked eye from the latitude 40°N. It appears to be a rich yellowish ...

  4. Category:Auriga - Wikipedia

    en.wikipedia.org/wiki/Category:Auriga

    3 Aur Other objects; Common name ... M 36: NGC 1960 M 37: NGC 2099 M 38: NGC 1912 Constellation map: Pages in category "Auriga" The following 155 pages are in this ...

  5. Psi3 Aurigae - Wikipedia

    en.wikipedia.org/wiki/Psi3_Aurigae

    This is a B-type giant star with a stellar classification of B8 III. [3] It has about 4.2 [ 7 ] and is spinning with a relatively high projected rotational velocity of 118 km/s. [ 8 ] The star is radiating 1,624 [ 6 ] times the Sun's luminosity from its photosphere at an effective temperature of 13,361 K. [ 8 ]

  6. List of stars in Auriga - Wikipedia

    en.wikipedia.org/wiki/List_of_stars_in_Auriga

    This is the list of notable stars in the constellation Auriga, sorted by decreasing brightness. Name B F Var HD HIP RA Dec vis. mag. abs. ... V min = 1.98 m, P = 3. ...

  7. AB Aurigae - Wikipedia

    en.wikipedia.org/wiki/AB_Aurigae

    AB Aurigae is a young Herbig Ae star [3] in the Auriga constellation. It is located at a distance of approximately 509 light years from the Sun based on stellar parallax. [1] This pre-main-sequence star has a stellar classification of A0Ve, [4] matching an A-type main-sequence star with emission lines in the spectrum.

  8. Beta Aurigae - Wikipedia

    en.wikipedia.org/wiki/Beta_Aurigae

    A light curve for Beta Aurigae, plotted from data published by Southworth et al. (2007) [3] Beta Aurigae is a binary star system, but it appears as a single star in the night sky. The two stars are metallic-lined subgiant stars belonging to the A-type stellar classification ; [ 3 ] they have roughly the same mass and radius.

  9. Iota Aurigae - Wikipedia

    en.wikipedia.org/wiki/Iota_Aurigae

    Iota Aurigae (ι Aurigae, abbreviated Iota Aur, ι Aur), officially named Hassaleh / ˈ h æ s ə l eɪ /, [12] is a star in the northern constellation of Auriga.It has an apparent visual magnitude of 2.7, [2] which is bright enough to be readily visible to the naked eye.