134 citations · 1.2k across the 51 of their papers we have counts for
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astro-ph.HE2011
Massive non-thermal radio emitters: new data and their modelling
D. Volpi, R. Blomme, M. De Becker +1
During recent years some non-thermal radio emitting OB stars have been discovered to be binary, or multiple systems. The non-thermal emission is due to synchrotron radiation that i…
astro-ph.SR2011★ 41 cited
The non-thermal radio emitter HD 93250 resolved by long baseline interferometry
H. Sana, J. -B. Le Bouquin, M. De Becker +3
As the brightest O-type X-ray source in the Carina nebula, HD 93250 (O4 III(fc)) is X-ray overluminous for its spectral type and has an unusually hard X-ray spectrum. Two different…