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astro-ph2006★ 31 cited
Non-thermal radio emission from O-type stars. II. HD 167971
R. Blomme, M. De Becker, M. C. Runacres +2
HD 167971 is a triple system consisting of a 3.3-day eclipsing binary (O5-8 V + O5-8 V) and an O8 supergiant. It is also a well known non-thermal radio emitter. We observed the rad…
astro-ph2006★ 36 cited
Can single O stars produce non-thermal radio emission?
S. Van Loo, M. C. Runacres, R. Blomme
We present a model for the non-thermal radio emission from presumably single O stars, in terms of synchrotron emission from relativistic electrons accelerated in wind-embedded shoc…