Pair production and non-thermal radio stars

Details Pair production and non-thermal radio stars Pair production and non-thermal radio stars

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aipc..101..433v&link_type=abstract

AIP Conference Proceedings, Volume 101, pp. 433-437 (1983).

Physics

Radio Sources, X-Ray Sources, X-Ray Bursts, Radiation Mechanisms, Polarization

Scientific paper

The generation of relativistic electrons and positrons in thermal
material surrounding a γ-ray source is examined. This in situ
generation of particles can resolve many of the problems associated with
the quiescent emission from non-thermal radio stars. The most luminous
radio star, Cyg X-3, is used as a paradigm throughout.

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