| |
 |
| 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 |
|
|
|
|
|
