Implications of the observed angular distribution of gamma-ray bursts for Galactic and cosmological models

Details Implications of the observed angular distribution of gamma-ray bursts for Galactic and cosmological models Implications of the observed angular distribution of gamma-ray bursts for Galactic and cosmological models

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..384..281l&link_type=abstract

Gamma-ray bursts: 3rd Huntsville symposium. AIP Conference Proceedings, Volume 384, pp. 281-290 (1996).

Mathematics

Logic

2

Gamma-Ray Sources, Gamma-Ray Bursts, Observational Cosmology, Astrometry And Reference Systems, Galactic Halo

Scientific paper

I consider the implications of the observed angular distribution of γ-ray bursts for Galactic and cosmological models of the bursts. The positions of individual bursts provide information about counterparts at other wavelengths. The angular distribution on small scales provides information about burst repetition. The angular distribution on intermediate scales constrains the distance scale to γ-ray bursts, if they are cosmological in origin. The angular distribution on large scales constrains Galactic corona models of the bursts. I discuss each of these topics in light of the BATSE 3B catalog.

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