Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2010-12-15
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
2 pages, 2 figures, poster at IAUS272
Scientific paper
Some OB stars show variable non-thermal radio emission. The non-thermal emission is due to synchrotron radiation that is emitted by electrons accelerated to high energies. The electron acceleration occurs at strong shocks created by the collision of radiatively-driven stellar winds in binary systems. Here we present results of our modelling of two colliding wind systems: Cyg OB2 No. 8A and Cyg OB2 No. 9.
Blomme Ronny
de Becker Michael
Rauw Gregor
Volpi Delia
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