Nova nucleosynthesis

被引：6
|
作者：
Starrfield, S
Truran, JW
Wiescher, M
Sparks, WM
机构：
[1] UNIV CHICAGO,DEPT ASTRON,CHICAGO,IL 60637
[2] UNIV CHICAGO,ENRICO FERMI INST,CHICAGO,IL 60637
[3] UNIV NOTRE DAME,DEPT PHYS,NOTRE DAME,IN 46556
[4] LOS ALAMOS NATL LAB,XNH,LOS ALAMOS,NM 87545
来源：
NUCLEAR PHYSICS A | 1997年 / 621卷 / 1-2期
关键词：
D O I：
10.1016/S0375-9474(97)00296-0
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：
We report on the results of hydrodynamic calculations, with updated nuclear reaction rates and opacities, which examine the consequences of the accretion process on 1.25M⊙ white dwarfs since that is the most probable mass for the white dwarf in V1974 Cyg 1992.
引用
收藏
页码：C495 / C498
页数：4
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