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[en] Explosive events in stars, especially supernovae, are expected to produce substantial quantities of short-lived radioactive isotopes as a part of the ongoing synthesis of heavy elements in the galaxy. Theoretically, the fluxes of γ rays produced by the decay of these distant nuclei should be detectable by experiments planned for the next decade. Observation of these signals will provide unique information regarding the ongoing chemical evolution of the galaxy and the nature of supernovae. (author)
Journal
Comments on Nuclear and Particle Physics; ISSN 0010-2709; 
; v. 9(6); p. 185-197
; v. 9(6); p. 185-197