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• W3099080975 abstract "We derive light curves for the hard γ-ray emission, at energies up to several TeV, expected from the unique pulsar/Be-star binary system PSR B1259-63. This is the only known system in our galaxy in which a radio pulsar is orbiting a main sequence star. We show that inverse Compton emission from the electrons and positrons in the shocked pulsar wind, scattering target photons from the Be star, produces a flux of hard γ-rays that should be above the sensitivity threshold of present day atmospheric Cerenkov detectors. Furthermore, we predict that the flux of hard γ-rays produced via this mechanism has a characteristic variation with orbital phase that should be observable, and which is not expected from any other mechanism" @default.
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• W3099080975 date "1999-01-01" @default.
• W3099080975 modified "2023-09-25" @default.
• W3099080975 title "Inverse Compton emission of TeV gamma rays from PSR B1259-63" @default.
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• W3099080975 doi "https://doi.org/10.1016/s0927-6505(98)00041-3" @default.
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