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

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dc.creatorPittard, J. M.
dc.date2009-05-20
dc.date.accessioned2026-07-07T13:16:50Z
dc.date.available2026-07-07T13:16:50Z
dc.descriptionThe 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.
dc.descriptionInvited review at HEPIMS Workshop (Jaen 2009); 12 pages, 5 figures, to appear in PASP
dc.identifierhttps://arxiv.org/abs/0905.3315
dc.identifierhttp://arxiv.org/abs/0905.3315
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/230917
dc.subjectHigh Energy Astrophysical Phenomena
dc.subjectSolar and Stellar Astrophysics
dc.titleModels of the non-thermal emission from early-type binaries
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