Modeling Gamma-Ray Emission From the High-Mass X-Ray Binary LS 5039

Modeling Gamma-Ray Emission From the High-Mass X-Ray Binary LS 5039

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. This paper focuses on the prominent γ-ray sour...

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Bibliographic Details
Main Authors:	Stan Owocki, Atsuo Okazaki, Gustavo Romero
Format:	Article
Language:	English
Published:	The Korean Space Science Society 2012-03-01
Series:	Journal of Astronomy and Space Sciences
Subjects:	X-rays: binaries gamma-rays: stars hydrodynamics
Online Access:	http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2012/v29n1/OJOOBS_2012_v29n1_51.pdf

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