AE Aurigae explained

AE Aurigae (abbreviated as AE Aur) is a runaway star in the constellation Auriga; it lights the Flaming Star Nebula.

Description

AE Aurigae is a blue O-type main sequence star with a mean apparent magnitude of +6.0. It is classified as an Orion type variable star and its brightness varies irregularly between magnitudes +5.78 and +6.08. It is approximately 1,300 light-years from Earth.

AE Aur is a runaway star that might have been ejected during a collision of two binary star groups. This collision, which also is credited with ejecting Mu Columbae and possibly 53 Arietis, has been traced to the Trapezium cluster in the Orion Nebula two million years ago. The binary Iota Orionis may have been the other half of this collision.[1]

AE Aur is seen to light up the Flaming Star nebula, but it was not formed within it. Instead it is passing through the nebula at high speed and producing a violent bow shock and high energy electromagnetic radiation.[2] [3]

Companions

Possibly due to its runaway star nature, AE Aurigae has no physical companion stars, although some nearby stars have been erroneously identified as ones. A theoretical companion 1000 AU (0.016 light-years) away from AE Aurigae would have an angular separation of less than 2.5 arcseconds and would probably be lost in the star's glare.

External links

Notes and References

  1. 2001A&A...365...49H. astro-ph/0010057. On the origin of the O and B-type stars with high velocities. II. Runaway stars and pulsars ejected from the nearby young stellar groups. Astronomy and Astrophysics. 365. 2. 49. Hoogerwerf. R.. De Bruijne. J. H. J.. De Zeeuw. P. T.. 2001. 10.1051/0004-6361:20000014. 18970167.
  2. 2012ApJ...757L...6L. 1208.6511. AE Aurigae: First Detection of Non-thermal X-Ray Emission from a Bow Shock Produced by a Runaway Star. The Astrophysical Journal Letters. 757. L6. López-Santiago. J.. Miceli. M.. Del Valle. M. V.. Romero. G. E.. Bonito. R.. Albacete-Colombo. J. F.. Pereira. V.. De Castro. E.. Damiani. F.. 2012. 1. 10.1088/2041-8205/757/1/L6. 37792833.
  3. 2007ApJ...655..920F. astro-ph/0610953. A Cometary Bow Shock and Mid-Infrared Emission Variations Revealed in Spitzer Observations of HD 34078 and IC 405. The Astrophysical Journal. 655. 2. 920–939. France. Kevin. McCandliss. Stephan R.. Lupu. Roxana E.. 2007. 10.1086/510481. 16963366.