The statistical properties of cosmic gamma-ray bursts

Details The statistical properties of cosmic gamma-ray bursts The statistical properties of cosmic gamma-ray bursts

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.164..277p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 164, no. 2, Feb. 1990, p. 277-283.

Astronomy and Astrophysics

Astrophysics

4

Cosmic Rays, Gamma Ray Bursts, Statistical Analysis, Milky Way Galaxy, Orion Constellation

Scientific paper

Recent localizations of cosmic gamma-ray bursts (GBRs) are studied taking into account the estimations of their intensities. The increase of the average intensity of GRBs along galactic longitudes of 220-260 and 40-80 deg is found. It may be associated with the Orion spiral arm and the central region of the Galaxy. Corresponding enhancement of the number of intense GRBs for directions along the Orion arm is also found. Astrophysical conclusions from this possible galaxy-scale distribution of GRBs are discussed.

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