Theoretical prediction of gamma-rays from SN 1991T

Details Theoretical prediction of gamma-rays from SN 1991T Theoretical prediction of gamma-rays from SN 1991T

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...97..223s&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 97, no. 1, p. 223, 224.

Astronomy and Astrophysics

Astronomy

9

Gamma Ray Astronomy, Gamma Ray Spectra, Stellar Evolution, Supernovae, Astronomical Spectroscopy, Light Curve, Radioactive Decay, Stellar Composition, Stellar Models

Scientific paper

We calculate the evolution of gamma-ray spectra from the recent unique
type Ia supernova SN 1991T based on the late detonation models. If a
similar supernova occurs at a distance not greater than 5 Mpc, gamma-ray
lines from the decays of Ni-56 and Co-56 in the outermost layers can be
observed with GRO significantly earlier than normal type Ia supernovae.

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