Close neutron star binaries

被引：0
|
作者：
Wilson, JR [1 ]
Mathews, GJ
Salmonson, JD
机构：
[1] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[2] Univ Notre Dame, Notre Dame, IN 46556 USA
来源：
NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS | 2002年 / 117卷 / 9-11期
关键词：
D O I：
暂无
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We present numerical hydrodynamic calculations of neutron star binaries. First we give results for binary stars in circular orbits and second we give results for stars in head-on collision. In both cases the stars undergo compression as they become closer together. In the first case of circular motion, the compression leads to a possible mechanism for gamma-ray bursts.
引用
收藏
页码：1257 / 1273
页数：17
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