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

页码：C495 / C498

页数：4

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