Gamma-ray bursts as standard-energy explosions

被引：84

作者：

Lipunov, VM

Postnov, KA

Prokhorov, ME

机构：

[1] Moscow MV Lomonosov State University, Sternberg Astron Inst, Moscow 119991, Russia

[2] Moscow MV Lomonosov State Univ, Moscow, Russia

来源：

ASTRONOMY REPORTS | 2001年 / 45卷 / 03期

基金：

俄罗斯基础研究基金会;

关键词：

D O I：

10.1134/1.1353364

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The distribution of observed energies for gamma-ray bursts with known redshifts can be explained as a consequence of events releasing a standard energy of E-0 = 5 x 10(51) erg. Two situations are possible: the degree of collimation could vary from burst to burst, or there could be a universal radiation pattern for all bursts, with the observed differences being due to differences in the orientation of this pattern relative to the line of sight to the Earth.

引用

页码：236 / 240

页数：5

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