Gamma-rays from the compact colliding wind region in Cyg OB2 #5
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🌌 astro-ph.HE
keywords
gamma-rayscollidingcompactproducedregionwindcontributiondetectability
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In this contribution we model the non-thermal emission (from radio to gamma-rays) produced in the compact (and recently detected) colliding wind region in the multiple stellar system Cyg OB2 #5. We focus our study on the detectability of the produced gamma-rays.
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