Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-03-23
Astronomy and Astrophysics
Astrophysics
To appear in the proceedings of "Massive Stars: Fundamental Parameters and Circumstellar Interactions"
Scientific paper
Massive WR+O star systems produce high-temperature, shock-heated plasma where the wind of the WR star and that of its binary companion collide - the wind-collision region (WCR). The WCR is a source of thermal (e.g. hard X-rays) and non-thermal (e.g. synchrotron) emission, the latter arising from electrons and ions accelerated to relativistic energies. These colliding wind binaries provide an excellent laboratory for the study of particle acceleration at higher mass, photon and magnetic energy densities than exist in SNRs. Recent models of the non-thermal emission from WR 140 have provided insight into this process.
Dougherty Sean M.
Pittard Julian Mark
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