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Supernova Abundance Generation

Published online by Cambridge University Press:  19 July 2016

K. Nomoto ,
T. Shigeyama  and
T. Tsujimoto
K. Nomoto
Affiliation:
Department of Astronomy, Faculty of Science, University of Tokyo, Tokyo 113
T. Shigeyama
Affiliation:
Department of Astronomy, Faculty of Science, University of Tokyo, Tokyo 113
T. Tsujimoto
Affiliation:
Department of Astronomy, Faculty of Science, University of Tokyo, Tokyo 113

Abstract

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Theoretical models of supernova explosions of various types are reviewed to obtain heavy element yields from supernovae. We focus on new models for SN 1987A, and Type Ia, Ib, and Ic supernovae. Maximum brightness and decline rate of their light curves suggest that 12–18 M⊙ stars produce larger amount of 56Ni than more massive stars. We discuss relative roles of various types of supernovae in the chemical evolution of galaxies.

Type
Setting the Stage
Information
Symposium - International Astronomical Union , Volume 145: Evolution of Stars: The Photospheric Abundance Connection , 1991 , pp. 21 - 38
Copyright
Copyright © Kluwer 1991 

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