Optical and gamma-ray bursts on neutron stars

Details Optical and gamma-ray bursts on neutron stars Optical and gamma-ray bursts on neutron stars

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63..984b&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 63, Sept.-Oct. 1986, p. 984-995. In Russian.

Astronomy and Astrophysics

Astronomy

4

Gamma Ray Bursts, Light Emission, Neutron Stars, Nuclear Fusion, Stellar Radiation, Iron, Nuclear Reactions, Stellar Flares, Thermal Plasmas

Scientific paper

γ-ray bursts are supposed to be connected with nuclear explosions under the surface of a neutron star due to chain reaction of fission of superheavy nuclei. Optical emission accompanying γ-ray bursts is produced by the expanding cloud of hot iron plasma illuminated by γ-ray emission of the neutron star. Parameters of the observed optical flash from the error box of 5 March 1979 are modelled theoretically and the estimate of the ratio Lopt/Lγ ≅ 5×10-4 is obtained.

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