Nearby stars as sources of gamma-ray bursts

被引:0
作者
P. D. Markin
B. I. Luchkov
机构
[1] National Research Nuclear University “MEPhI”,
来源
Bulletin of the Lebedev Physics Institute | 2014年 / 41卷
关键词
gamma astronomy; gamma-ray bursts; observations and sources of gamma-ray bursts; small-mass stars; nearby stars;
D O I
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中图分类号
学科分类号
摘要
Observations of ground-based telescopes and the Hubble space telescope made it possible to identify a part of gamma-ray bursts with far objects (redshift parameter Z ≥ 1).However, it remains unclear what are other bursts and what are their sources. The possibility of identifying other bursts with close sources known as small-mass flare stars is considered. The coordinates of space gamma-ray bursts (GRBs) for 2008–2013 and close stars (within the radius r < 25 pc) were compared by the correlation analysis method. Six coincidences were found with an accuracy of ∼0.1°. The probability of accidental coincidence of GRBs with stars is 4 · 10−8, which undoubtedly proves their stellar origin.
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页码:95 / 99
页数:4
相关论文
共 10 条
  • [1] Prilutskii O F(1975)undefined Usp. Fiz. Nauk 16 517-undefined
  • [2] Rozental I L(1996)undefined Usp. Fiz. Nauk 166 743-undefined
  • [3] Usov V V(1999)undefined Usp. Fiz. Nauk 169 545-undefined
  • [4] Luchkov B I(1997)undefined Nature 386 686-undefined
  • [5] Mitrofanov I G(2000)undefined Pisma Astron. Zh. 26 848-undefined
  • [6] Rozental I L(undefined)undefined undefined undefined undefined-undefined
  • [7] Postnov K A(undefined)undefined undefined undefined undefined-undefined
  • [8] van Paradijs P J(undefined)undefined undefined undefined undefined-undefined
  • [9] Groot S S(undefined)undefined undefined undefined undefined-undefined
  • [10] Gershtein undefined(undefined)undefined undefined undefined undefined-undefined