Gamma radiation expected from the supernova 1987A in the Large Magellanic Cloud

Details Gamma radiation expected from the supernova 1987A in the Large Magellanic Cloud Gamma radiation expected from the supernova 1987A in the Large Magellanic Cloud

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..744b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Sept. 1987, p. 744-750. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

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 0.1-3.5 MeV range escaping the SN 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 0.1-0.2 MeV and 0.8-0.9 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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