Results of multiyear observations of fluxes of superhigh-energy gamma-ray quanta from Cyg X-3

Details Results of multiyear observations of fluxes of superhigh-energy gamma-ray quanta from Cyg X-3 Results of multiyear observations of fluxes of superhigh-energy gamma-ray quanta from Cyg X-3

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982izssr..46.1665n&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Samarkand, Uzbek SSR, Oct. 27-29, 1981.) Akademiia Nauk SSSR, Izvestiia, Ser

Astronomy and Astrophysics

Astronomy

2

Energetic Particles, Gamma Ray Astronomy, Particle Flux Density, Annual Variations, Cygnus Constellation, X Ray Sources

Scientific paper

Regular observations of gamma rays of superhigh energies (exceeding 2 TeV) from Cyg X-3 were made at the Crimean Astrophysical Observatory from 1972 to 1980. A brief review of these observations indicates that the mean flux of gamma rays with energies exceeding 2 TeV amounted to (1.8 + or - 0.5) x 10 to the -11th quanta/sq cm s for the nine years. The mean flux during 1976-1979 was less than that during 1972-1975. The mean flux of the 4.8-hour periodic component for the nine years amounted to 1.3 x 10 to the -10th quanta/sq cm s.

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