Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...381..220a&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 381, Nov. 1, 1991, p. 220-227.
Astronomy and Astrophysics
Astrophysics
9
Gamma Ray Bursts, Pulsars, X Ray Binaries, Companion Stars, Stellar Models, Stellar Radiation
Scientific paper
A model of pulsed very high energy and ultrahigh energy gamma-radiation from X-ray binaries is proposed, which implies that the gamma-rays are due to the bombardment of a cloud ejected from the companion normal star by the relativistic proton beam stationarily accelerated by the pulsar. In the framework of this model all the peculiarities of the gamma-radiation observed from the X-ray binary Hercules X-1/HZ Herculis are naturally explained. The expected gamma-ray spectra in a wide energy range of E = 100 McV - 1 PeV, as well as the possibilities of experimental verification of the model proposed, are discussed.
Agaronian F. A.
Atoian A. M.
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