Publication Date:
2019-07-13
Description:
Most Galactic optical supernovae are hidden due to severe extinction in the disk, but could be detectable through their gamma-ray afterglow. Ti-44 is among the potentially detectable isotopes in supernova ejecta. HEAO 3 and SMM sky surveys have not detected gamma-ray lines from the decay of Ti-44, thus constraining SN rates and nucleosynthesis. We perform Monte Carlo simulations of the gamma-ray signatures of SN occurring during the last millenium to interpret the gamma-ray paucity.
Keywords:
ASTROPHYSICS
Type:
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138); 97; 1; p. 219, 220.
Format:
text
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