On gamma-ray bursts

Details On gamma-ray bursts On gamma-ray bursts

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977crasb.285..341d&link_type=abstract

Academie des Sciences (Paris), Comptes Rendus, Serie B - Sciences Physiques, vol. 285, no. 15, Nov. 28, 1977, p. 341-344. In Fr

Astronomy and Astrophysics

Astronomy

Binary Stars, Cosmic X Rays, Gamma Ray Astronomy, X Ray Sources, Annihilation Reactions, Astronomical Models, Dwarf Stars, Nuclear Reactions, Pulsars, Satellite Observation, Variable Stars

Scientific paper

Data from the Vela and Uhuru satellites are cited in arguing that gamma-ray bursts are most likely due to high-energy X-ray emissions from binary stars consisting of an eruptive dwarf star associated with a pulsar. Since the observed maximal energy of the bursts is less than 1.5 MeV, a nuclear origin for the gamma-ray emissions appears to be ruled out. Evidence related to such eruptive variables as the U Geminorum, T Tauri and UV Ceti stars, as well as novae, is mentioned in developing the argument.

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