Gamma radiation expected from supernova 1987A in large magellanic cloud

Details Gamma radiation expected from supernova 1987A in large magellanic cloud Gamma radiation expected from supernova 1987A in large magellanic cloud

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988rpsct....r..14b&link_type=abstract

In its JPRS Report: Science and Technology. USSR: Space p 14 (SEE N88-30498 24-88) Transl. into ENGLISH from Pisma v Astonomiche

Astronomy and Astrophysics

Astronomy

Gamma Ray Astronomy, Magellanic Clouds, Supernovae, Cobalt Isotopes, Monte Carlo Method, Pulsars, Stellar Envelopes

Scientific paper

The Monte Carlo method is used to obtain the spectra of photons in the 0.1 to 3.5 MeV range escaping the supernova 1987A envelope: they were generated during Co-56 decay or by the young pulsar. The time dependence of the gamma-flux in energy intervals of 0.1 to 0.2 MeV and 0.8 to 0.9 MeV is analyzed for variants of Co-56 decay. It is shown how differences in the parameters of the expanding envelope appear in the observations.

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