Interpretation of double structure in the celestial γ-ray bursts

Details Interpretation of double structure in the celestial γ-ray bursts Interpretation of double structure in the celestial γ-ray bursts

Jun 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974natur.249..747j&link_type=abstract

Nature, Volume 249, Issue 5459, pp. 747-748 (1974).

Physics

3

Scientific paper

THE essentially isotropic distribution of the Vela satellite γ-ray bursts1 implies that the sources are either very local and galactic, or very remote and extragalactic. Of the theories for a remote origin there are two schools of thought, either that these γ-rays originate in shock waves during the formation of type II supernovae2 or that they represent transient pulses of blackbody emission associated with the collapse of a white dwarf to a neutron star3.

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