Cosmic gamma-ray bursts

Details Cosmic gamma-ray bursts Cosmic gamma-ray bursts

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ssrv...36..319v&link_type=abstract

(International Astronomical Union, Meeting on Galactic Astrophysics and Gamma-Ray Astronomy, Patras, Greece, Aug. 19, 1982) Spac

Astronomy and Astrophysics

Astrophysics

3

Energy Spectra, Gamma Ray Bursts, Spatial Distribution, Astronomical Models, Particle Energy, Temporal Distribution

Scientific paper

The observational characteristics of gamma-ray bursts are reviewed, concerning their spectra as well as their temporal structure and spatial distribution. From this data, it is suggested that the sources belong to a thick halo population (scale height greater than 3 kpc), and that the mean recurrence time for one source is greater than 5 yr. The implications of these results are discussed, concerning the future experimental perspectives of detection of gamma-ray bursts, and also the constraints on theoretical models.

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