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Showing 1 to 1 of 1 for “"Colliding Wind Binary"”.
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Multidimensional diffusive shock acceleration in the Winds from massive stars
Nonthermal radio emission has been seen in the winds around a quarter of all O-stars. The emission is attributed to shock accelerated cosmic rays. The shocks thought to be causing the acceleration are either wind-embedded shocks due to radiative line driving instabilities in the stellar wind, or …