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 source,...
Guardado en:
| Autores principales: | Owocki, Stan, Okazaki, Atsuo, Romero, Gustavo Esteban |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2012
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84679 |
| Aporte de: |
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