Supernovae-Optical Precursors of Short Gamma-Ray Bursts

被引:3
作者
Dokuchaev, V. I. [1 ]
Eroshenko, Yu. N. [1 ]
机构
[1] Russian Acad Sci, Inst Nucl Res, Moscow 117319, Russia
来源
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2011年 / 37卷 / 02期
关键词
gamma-ray bursts; neutron stars; black holes; supernovae; NEUTRON-STAR; GRAVITATIONAL-WAVES; BLACK-HOLES; BINARY; COALESCENCE; EXPLOSION; DYNAMICS; COLLAPSE;
D O I
10.1134/S1063773710120035
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The probability of observing "supernova-gamma-ray burst" (GRB) pair events and recurrent GRBs from one galaxy in a time interval of several years has been estimated. Supernova explosions in binary systems accompanied by the formation of a short-lived pair of compact objects can be the sources of such events. If a short GRB is generated during the collision of a pair, then approximately each of similar to 300 short GRBs with redshift z must have an optical precursor-a supernova in the observer's time interval < 2(1 + z) yr. If the supernova explosion has the pattern of a hypernova, then a successive observation of long and short GRBs is possible. The scenario for the generation of multiple GRBs in collapsing galactic nuclei is also discussed.
引用
收藏
页码:83 / 90
页数:8
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