Back to Volume
Paper: Radio Observations of Mass Loss in OB Stars
Volume: 388, Mass Loss from Stars and the Evolution of Stellar Clusters
Page: 145
Authors: Blomme, R.
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.145
Back to Volume