Radio Observations of Mass Loss in OB Stars

Details Radio Observations of Mass Loss in OB Stars Radio Observations of Mass Loss in OB Stars

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..145b&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

Scientific paper

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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