GRAVITATIONAL WAVES VERSUS X-RAY AND GAMMA-RAY EMISSION IN A SHORT GAMMA-RAY BURST

被引：9
|
作者：
Oliveira, F. G. [1 ,2 ,3 ]
Rueda, Jorge A. [1 ,2 ,3 ]
Ruffini, R. [1 ,2 ,3 ]
机构：
[1] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy
[2] Univ Roma La Sapienza, ICRA, I-00185 Rome, Italy
[3] ICRANet, I-65122 Pescara, Italy
来源：
ASTROPHYSICAL JOURNAL | 2014年 / 787卷 / 02期
关键词：
binaries: close; equation of state; gamma-ray burst: individual (GRB 090227B); gravitational waves; stars: neutron; MEAN-FIELD THEORY; NEUTRON-STAR; SHORT GRB; AFTERGLOWS; NUCLEI; SYSTEM; CRUST;
D O I：
10.1088/0004-637X/787/2/150
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Recent progress in the understanding of the physical nature of neutron star equilibrium configurations and the first observational evidence of a genuinely short gamma-ray burst (GRB), GRB 090227B, allows us to give an estimate of the gravitational waves versus the X-ray and gamma-ray emission in a short GRB.
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页数：8
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