Nearby stars as sources of gamma-ray bursts

被引:0
|
作者
Markin, P. D. [1 ]
Luchkov, B. I. [1 ]
机构
[1] Natl Res Nucl Univ MEPhI, Moscow 115409, Russia
关键词
gamma astronomy; gamma-ray bursts; observations and sources of gamma-ray bursts; small-mass stars; nearby stars;
D O I
10.3103/S1068335614040022
中图分类号
O4 [物理学];
学科分类号
0702 ;
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 a parts per thousand yen 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 similar to 0.1A degrees. The probability of accidental coincidence of GRBs with stars is 4 center dot 10(-8), which undoubtedly proves their stellar origin.
引用
收藏
页码:95 / 99
页数:5
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