Gamma-rays from the compact colliding wind region in Cyg OB2 #5
arXiv:1210.3080 · doi:10.1063/1.4772287
Abstract
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.
arXiv commentTo appear in the proceedings of the 5th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma2012), held in Heidelberg, July 9-13, 2012