Possible Episodic Gamma-Ray Sources. Moving Fragile Target Crosses Relativistic Particle Beam

Details Possible Episodic Gamma-Ray Sources. Moving Fragile Target Crosses Relativistic Particle Beam Possible Episodic Gamma-Ray Sources. Moving Fragile Target Crosses Relativistic Particle Beam

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ssrv...75..357a&link_type=abstract

Space Science Reviews, Volume 75, Issue 1-2, pp. 357-373

Physics

13

Scientific paper

A model for production of episodic γ-ray event at interaction of a moving gas target with, a beam of relativistic particles is proposed. The typical duration of γ-ray emission is limited by the flight time of the target across the beam as well as by the time of destruction and/or expulsion of the target by luminous beam. The time-dependent radiation spectra of the expanding and moving gas cloud irradiated by the beam are calculated for the galactic binary systems Her X-1 and AE Aquarii which are reported as episodic γ-ray emitters at very high energies. Some predictions and observational tests for the model are discussed.

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