Nuclear gamma ray lines from supernovae

Details Nuclear gamma ray lines from supernovae Nuclear gamma ray lines from supernovae

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8026254j&link_type=abstract

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Gamma Rays, Line Spectra, Supernovae, Balloon Flight, Flux (Rate), Stratosphere, Telescopes

Scientific paper

From theoretical observations of the behavior of gamma ray lines fluxes occurring after a supernova explosion, the 1.156 and 0.847 MeV lines are seen to be the most likely to be observed. The 1.156 MeV line was previously observed by other investigators. Observations are reported of the 0.847 MeV line, and 1,332, 1.173 and 0.059 MeV lines using a Ge(Li) telescope aboard a stratospheric balloon which was flown in Brazil in 1977. The observation using a NaI(Tl) detector of a line in the energy interval 1.5 - 1.6 MeV is also reported. It may be due to O18 (p, p prime) O18* reaction.

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