C. R. KertonChristopher M. BruntC. E. JonesShantanu Basu
The jets of microquasars with high-mass stellar companions are exposed to the dense matter field of the stellar wind.We present estimates of the gamma-ray emission expected from the jet-wind hadronic interaction and we discuss the detectability of the phenomenon at high energies.The proposed mechanism could explain some of the unidentified gamma-ray sources detected by EGRET instrument on the galactic plane.
C. R. KertonC. M. BruntC. E. JonesS. Basu