CYG X-3, an ultrahigh-energy gamma pulsar with a period of 9.22 MS

Details CYG X-3, an ultrahigh-energy gamma pulsar with a period of 9.22 MS CYG X-3, an ultrahigh-energy gamma pulsar with a period of 9.22 MS

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2325z&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

3

Cygnus Constellation, Gamma Rays, High Energy Interactions, Pulsars, Electromagnetic Radiation, Pulse Duration

Scientific paper

An examination of experimental data indicates that Cyg X-3 contains a pulsar rotating with a period of 99.22090 ms (on September 28, 1978) and radiating ultrahigh-energy gamma rays. The gamma flux with an energy exceeding 10 to the 12th eV in a pulse is equal to 2 x 10 to the -11th/sq cm s; the period-averaged flux is 1.3 x 10 to the -11th/sq cm s.

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