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A model for gamma-ray binaries, based on the effect of pair production feedback in shocked pulsar winds
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A model for gamma-ray binaries, based on the effect of pair production feedback in shocked pulsar winds
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We analyze the model of gamma-ray binaries, consisting of a massive star and a pulsar with ultrarelativistic wind. We consider radiation from energetic particles, accelerated at the pulsar wind termination shock, and feedback of this radiation on the wind through production of secondary electron-positron pairs. We show that the pair feedback limits the Lorentz factor of the pulsar wind and creates a population of very energetic pairs, whose radiation may be responsible for the observed gamma-ray signal.
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Cited by 1 Pith paper
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Large-scale emission from gamma-ray binaries: the case of LS 5039
The arcminute X-ray emission around LS 5039 is consistently explained as synchrotron radiation from electrons accelerated at the termination shock of the mixed stellar/pulsar wind, with different source ages giving co...
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