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AE Aurigae

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IC 405 (also known as the Flaming Star Nebula, SH 2-229, or Caldwell 31) is an emission and reflection nebula in the constellation Auriga, surrounding the bluish star AE Aurigae.
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It is thought to have originated in a supernova explosion about 2 million years ago, which may have also created several known runaway stars, including AE Aurigae, Mu Columbae and 53 Arietis, which are believed to have been part of a multiple star system in which one component exploded as a supernova.
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Its red, convoluted clouds of glowing hydrogen gas are energized by hot O-type star AE Aurigae.
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AE Aurigae - Wikipedia, the free encyclopedia
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in the constellation Auriga and owes its name to the variable star AE Aurigae, to give the impression that is burning.
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It turns out that WISE is particularly adept at imaging bow shocks from runaway stars. Previous examples can be seen around Zeta Ophiuchi, AE Aurigae, and Menkhib.
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IC405, The Flamingstar nebulac ontains a cloud of hidrogene that shines excited by the ultraviolet radiation of the runaway star "AE Auriga" (moves at 200km/s and comes from the Orion Nebula).
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IC405, The Flamingstar nebula can be seen in the right area of the image. Contains a cloud of hidrogene that shines excited by the ultraviolet radiation of the runaway star "AE Auriga" (moves at 200km/s and comes from the Orion Nebula).
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One example of a related set of runaway stars is the case of AE Aurigae, 53 Arietis and Mu Columbae, all of which are moving away from each other at velocities of over 100 km/s (for comparison, the Sun moves through the Milky Way at about 20 km/s faster than the local average).
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Results. From our analysis, we confirm that the X-ray emission from the bow shock produced by AE Aurigae can be explained by inverse Compton processes involving the infrared photons of the heated dust. We also predict low high-energy flux emission from the bow shock produced by BD+43 3654, and the possibility of high-energy emission from the bow shock formed by a supergiant star during the transition phase from blue to red supergiant.
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