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...

Ausführliche Beschreibung

Bibliographische Detailangaben
Hauptverfasser: Stan Owocki, Atsuo Okazaki, Gustavo Romero
Format: Artikel
Sprache:English
Veröffentlicht: The Korean Space Science Society 2012-03-01
Schriftenreihe:Journal of Astronomy and Space Sciences
Schlagworte:
Online Zugang:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2012/v29n1/OJOOBS_2012_v29n1_51.pdf