A search for supernovae preceding short gamma-ray bursts

被引:0
作者
V. I. Dokuchaev
Yu. N. Eroshenko
机构
[1] Institute for Nuclear Research of the Russian Academy of Sciences,
来源
Gravitation and Cosmology | 2012年 / 18卷
关键词
Black Hole; Neutron Star; Compact Object; Supernova Explosion; Population Synthesis;
D O I
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学科分类号
摘要
We have found the probability of double events “supernova—gamma-ray burst” (GRB) separated by a time interval of a few years. Their sources can be supernova explosions in binary systems accompanied by formation of a short-lived pair of compact objects which produce a short GRB while merging. Each of the ∼500 short SGBs must have an optical precursor, a supernova at a time interval of < 2 years. We discuss the possible relationship between SN 1997ds and GRB 990425.
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页码:97 / 99
页数:2
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共 11 条
  • [1] Blinnikov S. I.(1984)undefined Pis’ma v AZh 10 422-undefined
  • [2] Paczynski B.(1986)undefined Astrophys. J. 308 L43-undefined
  • [3] Hills J.G.(1983)undefined Astrophys. J 267 322-undefined
  • [4] Grishchuk L. P.(2001)undefined Usp. Fiz. Nauk 171 3-undefined
  • [5] Piran T.(2004)undefined Rev. Mod. Phys. 76 1143-undefined
  • [6] Dokuchaev V. I.(2011)undefined Astron. Lett. 37 83-undefined
  • [7] Eroshenko Yu. N.(2001)undefined Astrophys. J. 563 80-undefined
  • [8] Stern B. E.(2001)undefined PASP 113 920-undefined
  • [9] Leonard D. C.(2010)undefined Mon. Not. Roy. Astron. Soc. 401 1381-undefined
  • [10] Filippenko A. V.(undefined)undefined undefined undefined undefined-undefined