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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 ...
File:Auriga_constellation_map.png licensed with Cc-by-sa-3.0-migrated, GFDL 2004-12-12T17:53:02Z Alfio 2559x2559 (280768 Bytes) Auriga constellation map (bigger image) 2004-12-12T12:12:04Z Alfio 427x427 (28366 Bytes) Auriga constellation map
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 ...
Animated 3D map of the nearest stars, ... flare star Epsilon Indi ... Gliese 268 (Ross 986, QY Aurigae) A 19.7414
EO Aurigae is an eclipsing binary of Algol type in the northern constellation of Auriga. With a combined apparent magnitude of 7.71, [ 3 ] it is too faint to be seen with the unaided eye. The eclipsing binary nature of the star was detected in 1943 by Sergei Gaposchkin at Harvard College Observatory . [ 7 ]
AE Aurigae is a blue O-type main sequence star with a mean apparent magnitude of +6.0, making it faintly visible to the naked eye under very good observing conditions. It was discovered to be a variable star by Daniel Walter Morehouse , in 1923, and received its variable star designation in 1924. [ 9 ]
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Upsilon Aurigae, Latinised from υ Aurigae, is the Bayer designation for a single [11] star in the northern constellation of Auriga. It has an apparent visual magnitude of 4.74, [2] which means it is bright enough to be seen with the naked eye. Based upon parallax measurements, this star is approximately 500 light-years (150 parsecs) distant ...
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