Observations of the gamma-quantum source Cygnus X-3 in 1989 at the GT-48 installation

Details Observations of the gamma-quantum source Cygnus X-3 in 1989 at the GT-48 installation Observations of the gamma-quantum source Cygnus X-3 in 1989 at the GT-48 installation

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.2045v&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, Russia, Nov. 1-3, 1990, Materialy. A92-40776 16-93) Akademiia Nauk

Astronomy and Astrophysics

Astronomy

1

Cygnus Constellation, Proton Flux Density, Stellar Flares, X Ray Sources, Energy Spectra, Gamma Ray Astronomy, X Ray Astronomy

Scientific paper

Observations of the X-ray source Cyg X - 3 beginning in July 1989 are reported. The separation of flares initiated by protons from flares caused by gamma-quanta with energy greater than 10 exp 12 eV was conducted by the main component method. The light curve for a period of 4.8 hr is consistent with an earlier curve for a period derivative value of 2.4 x 10 exp -9 s/s.

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