Radioactive Nuclei from Type IA Supernovae

Details Radioactive Nuclei from Type IA Supernovae Radioactive Nuclei from Type IA Supernovae

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.203k&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

X- and gamma-ray emission from supernovae originates mostly from radioactive decays of 56Ni 56Co 56Fe sequence. The predicted emission from standard SNe Ia is relatively strong compared with other types of supernovae because of their smaller ejecta mass and larger 56Ni mass. For the peculiar SNe Ia such as SN 1991T, optical observations suggest the existence of 56Ni in the outer layers, which means more intense line gamma-ray emission than standard SNe Ia.

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