Modeling Gamma-Ray Emission From the High-Mass X-Ray Binary LS 5039 by Stan Owocki, Atsuo Okazaki, Gustavo Romero

“…A few high-mass X-ray binaries–consisting of an OB star plus compact companion– have been observed by Fermi and ground-based Cerenkov telescopes like High Energy Stereoscopic System (HESS) to be sources of very high energy (VHE; up to 30 TeV) γ-rays. …”
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