Low-Mass Neutron Stars with Rotation

被引：9
|
作者：
Yudin, A., V [1 ,2 ]
Razinkova, T. L. [1 ]
Blinnikov, S., I [1 ,3 ]
机构：
[1] Inst Theoret & Expt Phys, Ul Bolshaya Cheremushkinskaya 25, Moscow 117259, Russia
[2] Natl Res Ctr, Kurchatov Inst, Pl Kurchatova 1, Moscow 123182, Russia
[3] Univ Tokyo, Kashizoa WPI, Kavli IPMU, Tokyo, Japan
来源：
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2019年 / 45卷 / 12期
基金：
俄罗斯基础研究基金会;
关键词：
low-mass neutron stars; binary systems; stellar rotation; MINIMUM MASS; EQUATION; EXPLOSION; STATE;
D O I：
10.1134/S1063773719120077
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The properties of low-mass neutron stars with rigid rotation are considered. The possible evolution paths of such stars in a close binary system with mass transfer are calculated. The properties of the gamma-ray burst GRB 170817A interpreted in terms of the stripping model, a natural ingredient of which is the explosion of a low-mass neutron star-a binary component, are briefly discussed.
引用
收藏
页码：847 / 854
页数：8
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