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  2. Epsilon Aurigae - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Aurigae

    Epsilon AurigaeAurigae, 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. Category:Auriga - Wikipedia

    en.wikipedia.org/wiki/Category:Auriga

    Constellation map Pages in category "Auriga" ... List of stars in Auriga; 0–9. 1 Aurigae; 2 Aurigae; 3C 147; 4C +41.17; 5 Aurigae; ... Epsilon Aurigae; Eta Aurigae ...

  4. Category:B-type main-sequence stars - Wikipedia

    en.wikipedia.org/wiki/Category:B-type_main...

    B-type main-sequence stars are main-sequence stars (luminosity class V) of spectral type B. Wikimedia Commons has media related to Blue-white dwarfs . Contents

  5. List of nearest stars by spectral type - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars_by...

    It is the 2nd/3rd nearest individual star to the Solar System, and the fourth-brightest individual star in the night sky. Has one candidate exoplanet. Tau Ceti: 11.912 ± 0.007: G8V [76] 0.793 ± 0.004 [120] [121] 0.800 ± 0.008 [121] 3.5 [120] 5.68 [120] Also the 20nd nearest star system to the Solar System. Eta Cassiopeiae A (Achird) 19.42 ...

  6. Category:F-type main-sequence stars - Wikipedia

    en.wikipedia.org/wiki/Category:F-type_main...

    Pages in category "F-type main-sequence stars" The following 200 pages are in this category, out of approximately 500 total. This list may not reflect recent changes .

  7. List of largest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_largest_stars

    Other methods can use lunar occultations or from eclipsing binaries, which can be used to test indirect methods of finding stellar radii. Only a few supergiants can be occulted by the Moon, including Antares and 119 Tauri. Examples of eclipsing binaries are Epsilon Aurigae (Almaaz), VV Cephei, and V766 Centauri (HR 5171).

  8. Algol variable - Wikipedia

    en.wikipedia.org/wiki/Algol_variable

    Algol variables or Algol-type binaries are a class of eclipsing binary stars that are similar to the prototype member of this class, β Persei (Beta Persei, Algol). An Algol binary is a system where both stars are near-spherical such that the timing of the start and end of the eclipses is well-defined.

  9. Capella - Wikipedia

    en.wikipedia.org/wiki/Capella

    A few degrees to the southwest of Capella lie three stars, Epsilon Aurigae, Zeta Aurigae and Eta Aurigae, the latter two of which are known as "The Kids", or Haedi. The four form a familiar pattern, or asterism , in the sky.