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AE Aurigae: First detection of non-thermal X-ray emission from a bow shock produced by a runaway star

2012

Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow shocks have been detected in the mid-infrared for several high-mass runaway stars and in radio waves for one star. Theoretical models predict the production of high-energy photons by non-thermal radiative processes in a number sufficiently large to be detected in X-rays. To date, no stellar bow shock has been detected at such energies. We present the first detection of X-ray emission from a bow shock produced by a runaway star. The star is AE Aur, which was likely expelled from its birthplace due to the encounter of two massive binary systems and now is passing through the dense nebula IC 405…

Shock waveAstrofísicaCiencias Astronómicasstars: kinematics and dynamicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsX-rays: generalISM: cloudsmassive [stars]general [X-rays]Radiative transferISM: clouds radiation mechanisms: non-thermal stars: individual: AE Aur stars: kinematics and dynamics stars: massive X-rays: generalAstrophysics::Solar and Stellar AstrophysicsBow shock (aerodynamics)kinematics and dynamics [stars]Solar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsCosmic dustPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NebulaAstronomy and Astrophysicsradiation mechanisms: non-thermalnon-thermal [radiation mechanisms]Astrophysics - Astrophysics of GalaxiesInterstellar mediumAstronomíastars: individual (AE Aur)stars: massiveStarsindividual (AE Aur) [stars]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaclouds [ISM]Radio wave
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