Non-thermal radiation from single O stars

Details Non-thermal radiation from single O stars Non-thermal radiation from single O stars

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002jad.....8s...8v&link_type=abstract

The Journal of Astronomical Data, Vol. 8, 8H 2002

Astronomy and Astrophysics

Astronomy

Scientific paper

For some of the most luminous O stars non-thermal radio emission has been observed. It is understood that synchrotron radiation from relativistic particles can account for this emission. These particles are accelerated to such high energies by shocks in the wind. In this article we discuss the use of two different wind models for reproducing the observational data.

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