Physics
Scientific paper
Nov 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005mshe.work...61v&link_type=abstract
"Proceedings of "Massive Stars and High-Energy Emission in OB Associations", a workshop of the JENAM 2005, "Distant Worlds", hel
Physics
3
Scientific paper
We present qualitative models for the non-thermal radio emission of single O stars, in terms of synchrotron emission by wind-embedded shocks. When we include the fact that shocks weaken as they move out with the wind, as predicted by time-dependent hydrodynamical simulations, these models produce a radio spectrum with a positive slope (as function of frequency), in contradiction with the observed negative slope. We conclude that non-thermal radio emission cannot originate from wind-embedded shocks, and is likely to be caused by a wind-colliding shock. A radio light curve analysis of two non-thermal O stars that are generally assumed to be single supports this conclusion.
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