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Supernova Abundance Generation

  • K. Nomoto (a1), T. Shigeyama (a1) and T. Tsujimoto (a1)
Abstract

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.

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Copyright
COPYRIGHT: © Kluwer 1991 
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