Gamma-Bursts and Black Holes

被引：0
作者：
I.L. Rosental
I. Belousova
机构：
[1] Space Research Institute,
来源：
Astrophysics and Space Science | 1997年 / 252卷
关键词：
Black Hole; Total Energy; Compact Object; Cosmological Distance; Burst Intensity;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Cosmic gamma ray bursts (GRB) are assumed to occur at cosmological distances, and to accompany collisions of compact objects. In this case, the burst intensity recorded at the Earth can help determine the total energy of the burst in the source, and to infer the mass of the source. If the mass exceeds 5M⊙, it can be assumed that one of the sources is a black hole.
引用
收藏
页码：461 / 463
页数：2
相关论文
共 14 条
  • [1] Abell G.(1989)undefined Astrophys. J. Suppl. 70 2-undefined
  • [2] Gorwin H.(1992)undefined Science 256 325-undefined
  • [3] Olwin R.(1996)undefined Sov. Phys. Uspechi (on Russian) 166 809-undefined
  • [4] Abramovici A.(1996)undefined Astrophys. J. 467 L41-undefined
  • [5] Althouse W.(1993)undefined Astrophys. J. 388 L45-undefined
  • [6] Drever R.(1993)undefined Astrophys. J. 405 278-undefined
  • [7] Cherepashchuk A.(1991)undefined Acta Astronomica 41 257-undefined
  • [8] Kollat T.(undefined)undefined undefined undefined undefined-undefined
  • [9] Piran T.(undefined)undefined undefined undefined undefined-undefined
  • [10] Mao S.(undefined)undefined undefined undefined undefined-undefined
12