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Hydrodynamics and high-energy physics of Wolf-Rayet colliding winds
Published online by Cambridge University Press: 07 August 2017
Abstract
The stellar winds flowing out of the components of WR+OB binaries can collide and shock waves are formed. Stellar wind collision, particle acceleration by the shocks and generation of X-ray, γ-ray, radio and IR emission in WR+OB binaries are discussed.
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- Session VII - Hydrodynamics and high-energy physics of colliding winds
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- Copyright © Kluwer 1995
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