Gamma radiation from the central region of the galaxy and the search for flare activity at energy not less than 100 MeV

Details Gamma radiation from the central region of the galaxy and the search for flare activity at energy not less than 100 MeV Gamma radiation from the central region of the galaxy and the search for flare activity at energy not less than 100 MeV

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975izssr..39q.424b&link_type=abstract

(Mezhdunarodnyi Seminar po Uskoreniiu Chastits i Iadernykh Reaktsii v Kosmose, 6th, Leningrad, USSR, Aug. 19-21, 1974.) Akademii

Astronomy and Astrophysics

Astronomy

Galactic Nuclei, Galactic Radiation, Gamma Rays, X Ray Astronomy, Celestial Sphere, Flares, Radiant Flux Density, Radiation Sources, Regression Analysis, Satellite Observation, Statistical Analysis

Scientific paper

Results are presented for measurements of the gamma flux from the central region of the galaxy and an estimate of the upper limit on gamma-like flare activity in the celestial sphere. The experimental data consist of about 4000 gamma-like events detected in eight regions of the celestial sphere with a gamma telescope on board Cosmos 561. The central region is found to have an excess of gamma radiation on the order of about 0.12 in relation to the other regions. An upper limit of 33.55 sec is determined for the duration of gamma-like flares in all eight regions.

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