000002818 001__ 2818
000002818 005__ 20160701171711.0
000002818 0247_ $$2DOI$$a10.1017/S1743921311011689
000002818 037__ $$aASTROimport-975
000002818 100__ $$aVolpi, D.
000002818 245__ $$aNon-thermal radio emission from colliding-wind binaries: modelling Cyg OB2 No. 8A and No. 9
000002818 260__ $$c2011
000002818 520__ $$aSome OB stars show variable non-thermal radio emission. The non-thermal emission is due to synchrotron radiation that is emitted by electrons accelerated to high energies. The electron acceleration occurs at strong shocks created by the collision of radiatively-driven stellar winds in binary systems. Here we present results of our modelling of two colliding wind systems: Cyg OB2 No. 8A and Cyg OB2 No. 9. 
000002818 700__ $$a Blomme, R.
000002818 700__ $$a De Becker, M.
000002818 700__ $$a Rauw, G.
000002818 773__ $$c638-639$$pActive OB Stars: Structure, Evolution, Mass Loss, and Critical Limits$$v272$$y2011
000002818 85642 $$ahttp://esoads.eso.org/abs/2011IAUS..272..638V
000002818 905__ $$apublished in
000002818 980__ $$aNONREF