Nucleosynthesis in type II supernovae

被引：244

作者：

Nomoto, K

Hashimoto, M

Tsujimoto, T

Thielemann, FK

Kishimoto, N

Kubo, Y

Nakasato, N

机构：

[1] KYUSHU UNIV, FAC SCI, DEPT PHYS, FUKUOKA 810, JAPAN

[2] NATL ASTRON OBSERV, MITAKA, TOKYO 181, JAPAN

[3] UNIV BASEL, INST THEORET PHYS, CH-4056 BASEL, SWITZERLAND

来源：

NUCLEAR PHYSICS A | 1997年 / 616卷 / 1-2期

关键词：

D O I：

10.1016/S0375-9474(97)00076-6

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

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

引用

页码：C79 / C90

页数：12

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