000002572 001__ 2572
000002572 005__ 20160701171707.0
000002572 037__ $$aASTROimport-729
000002572 100__ $$aBlomme, R.
000002572 245__ $$aRadio Observations of Mass Loss in OB Stars
000002572 260__ $$c2008
000002572 520__ $$aRadio fluxes of OB stars can be dominated by either thermal or non-thermal emission. Thermal radiation can be used to study clumping in the wind. Non-thermal radiation is a signature of colliding winds in a binary system. 
000002572 773__ $$c145$$pMass Loss from Stars and the Evolution of Stellar Clusters$$v388$$y2008
000002572 85642 $$ahttp://esoads.eso.org/abs/2008ASPC..388..145B
000002572 905__ $$apublished in
000002572 980__ $$aNONREF