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The jets of microquasars with high-mass stellar companions are exposed to thedense matter field of the stellar wind. We present estimates of the gamma-rayemission expected from the jet-wind hadronic interaction and we discuss thedetectability of the phenomenon at high energies. The proposed mechanism couldexplain some of the unidentified gamma-ray sources detected by EGRET instrumenton the galactic plane.Comment: Accepted for publication in Astronomy and Astrophysics as a Letter to  the Edito

Hadronic gamma-ray emission from windy microquasars