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published in Mass Loss from Stars and the Evolution of Stellar Clusters, 388, pp. 145 (2008)
Abstract: Radio fluxes of OB stars can be dominated by either thermal or non-thermal emission. Thermal radiation can be used to study clumping in the wind. Non-thermal radiation is a signature of colliding winds in a binary system.
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Royal Observatory of Belgium > Astronomy & Astrophysics
Science Articles > Non-refereed Articles