Models of the non-thermal emission from early-type binaries

J. M. Pittard

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arXiv · 0905.3315

Models of the non-thermal emission from early-type binaries

J. M. Pittard

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Abstract

The powerful wind-wind collision in massive star binaries creates a region of high temperature plasma and accelerates particles to relativistic energies. I briefly summarize the hydrodynamics of the wind-wind interaction and the observational evidence, including recent $γ$-ray detections, of non-thermal emission from such systems. I then discuss existing models of the non-thermal emission and their application to date, before concluding with some future prospects.

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J. M. Pittard. 2009-05-20. Models of the non-thermal emission from early-type binaries. https://arxiv.org/abs/0905.3315

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