Cherenkov Telescope results on gamma-ray binaries
作者： Juan Cortina
DOI:
关键词: Cherenkov radiation 、 Astronomy 、 Telescope 、 Phenomenology (particle physics) 、 Particle acceleration 、 Pulsar 、 High energy 、 Binary number 、 Physics 、 Astrophysics 、 Gamma ray
摘要: In the past ten years of regular operations, a new generation Cherenkov telescopes have established binary systems as class Very High Energy gamma-ray (VHE) emitters. Particle acceleration in these may occur either an accretion-powered jet (microquasar) or shock between pulsar wind and stellar (wind-wind). This paper describes phenomenology three VHE binaries PSR~B1259-63, LS 5039 I +61 303. Two other objects belong to this class: HESS J0632+057 is point-like variable source whose multiwavelength behaviour resembles that binaries, whereas Cyg X-1 well-known accreting system which been detected during flaring episode. The concludes with review latest searches for telescopes, special emphasis on X-3.
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arxiv.org参考文章(45)
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