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Supernova Nucleosynthesis in Massive Stars

Published online by Cambridge University Press:  12 April 2016

M. Hashimoto ,
K. Nomoto ,
T. Tsujimoto  and
F.-K. Thielemann
M. Hashimoto
Affiliation:
Kyushu University, Fukuoka 810, Japan
K. Nomoto
Affiliation:
University of Tokyo, Bunkyo-ku, Tokyo 113, Japan
F.-K. Thielemann
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA

Abstract

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Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 Mʘ to 70 Mʘ are calculated. We examine the dependence of the supernova yields on the stellar mass, 12C(α, γ)16O rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.

Type
Type lb and Type II Supernovae
Information
International Astronomical Union Colloquium , Volume 145: Supernovae and Supernova Remnants , 1996 , pp. 157 - 164
Copyright
Copyright © Cambridge University Press 1996

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