Binary star model of the gamma-ray burst with special reference to that on 5 March, 1979 and subsequent bursts on 6 March, 4 April, and 24 April, 1979

Details Binary star model of the gamma-ray burst with special reference to that on 5 March, 1979 and subsequent bursts on 6 March, 4 April, and 24 April, 1979 Binary star model of the gamma-ray burst with special reference to that on 5 March, 1979 and subsequent bursts on 6 March, 4 April, and 24 April, 1979

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.102..235s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 102, no. 2, July 1984, p. 235-245.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Gamma Ray Bursts, Stellar Evolution, Stellar Mass Accretion, Stellar Models, Gravitational Collapse, Neutron Stars, Nuclear Fusion, Stellar Composition, X Rays

Scientific paper

The peculiar v-ray burst phenomenon of 5 March, 1979, and the other subsequent bursts on 6 March, 4 April, and 24 April, 1979, are studied, using the physically more realistic exponentially increasing accretion rate on a highly magnetized neutron star from its companion, and the conclusions that pycno- nuclear reaction flash for the first and thermonuclear flashes for the subsequent bursts as the most probable model for this series of bursts, are made. We further conclude that a huge y-ray burst is a sequel to rapid X-ray transient or type-I X-ray bursts, i.e., an almost exactly similar burst as on 5 April, 1979 will never repeat from the same source, instead rapid X-ray transient burst, or type-I X-ray burst will be occured. A rough estimate gives that the next burst will occur within 0.5 yr since 24 April, 1979

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