Gamma nuclear lines produced in supernovae and the possibility of detection

Details Gamma nuclear lines produced in supernovae and the possibility of detection Gamma nuclear lines produced in supernovae and the possibility of detection

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...7934154j&link_type=abstract

Presented at the 31th Reuniao Annual da Soc. Brasil. para o Progr. da Cienc. (SBPC), 11-18 Jul. 1979

Astronomy and Astrophysics

Astrophysics

Galaxies, Gamma Rays, Nuclear Fusion, Nuclear Interactions, Supernovae, Astrophysics, Atomic Weights, Line Spectra, Nuclear Scattering

Scientific paper

The nuclear fusion reaction which results in the origin of a supernova is studied. These explosive nuclear synthesis occur between two elements of atomic weights between 28 and 57 as well as in reactions produced by high energy particles surrounded by gas. In the Galaxy N6C5236 the nuclear Gamma lines are best observed, since there are more of these phenomenons occuring there.

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