Observation of Cyg X-3 in the primary gamma-ray energy range greater than about 10 to the 14th eV

Details Observation of Cyg X-3 in the primary gamma-ray energy range greater than about 10 to the 14th eV Observation of Cyg X-3 in the primary gamma-ray energy range greater than about 10 to the 14th eV

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987izssr..51.1768a&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 51, Oct. 1987, p. 1768-1771. In Russian.

Astronomy and Astrophysics

Astronomy

Energetic Particles, Gamma Ray Astronomy, X Ray Binaries, Cosmic Ray Showers, Flux Quantization, Phase Deviation, Radiation Sources

Scientific paper

The paper examines observations of Cyg X-3 at primary gamma-ray energies exceeding 10 to the 14 eV made with the Kover facility of the Baksan neutrino observatory from July 1, 1984 to June 30, 1985. Phase curves for the Cyg X-3 cell are presented, and ultrahigh-energy gamma-ray fluxes are assessed according to data from various experimental facilities.

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