Possible models for the high-energy transient GB790107

Details Possible models for the high-energy transient GB790107 Possible models for the high-energy transient GB790107

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987natur.327..398l&link_type=abstract

Nature (ISSN 0028-0836), vol. 327, June 4, 1987, p. 398-400. NSF-NASA-supported research.

Physics

11

Astronomical Models, Gamma Ray Bursts, Neutron Stars, Stellar Envelopes, Stellar Physics, Transient Response

Scientific paper

The discovery of rapid repetitive soft γ-ray burst events on timescales as short as seconds from GB790107 may have important implications for our understanding of the γ-ray burst mechanism. The properties of GB790107 place severe constraints on the viability of models proposed for the typical γ-ray burst events as applied to this soft γ-ray repeater. The authors review the various models proposed for γ-ray bursts and show that a model involving a comet cloud around a neutron star is consistent with the observational data.

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