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- W3026158732 abstract "In the past ten years of regular operations, a new generation of Cherenkov telescopes have established binary systems as a new class of Very High Energy γ- ray (VHE) emitters. Particle acceleration in these systems may occur either in an accretion-powered jet (“microquasar”) or in the shock between a pulsar wind and a stellar wind (“wind-wind”). This paper describes the phenomenology of the three VHE binaries PSR B1259-63, LS 5039 and LS I+61?303. Two other objects may belong to this new class: HESS J0632+057 is a point-like variable VHE source whose multiwavelength behaviour resembles that of the other binaries, whereas Cyg X-1 is a well-known accreting system which may have been detected in VHE during a flaring episode. The paper concludes with a review of the latest searches for other binaries with Cherenkov telescopes, with special emphasis on Cyg X-3." @default.
- W3026158732 created "2020-05-29" @default.
- W3026158732 creator A5065046115 @default.
- W3026158732 date "2010-12-14" @default.
- W3026158732 modified "2023-10-08" @default.
- W3026158732 title "Cherenkov Telescope results on gamma-ray binaries" @default.
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- W3026158732 doi "https://doi.org/10.1007/978-3-642-17251-9_42" @default.
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