Giant shells and stellar arcs as relics of gamma-ray burst explosions

被引：36

作者：

Efremov, YN

Elmegreen, BG

Hodge, PW

机构：

[1] Moscow MV Lomonosov State Univ, Sternberg State Astron Inst, Moscow 119899, Russia

[2] IBM Corp, Thomas J Watson Res Ctr, Yorktown Hts, NY 10598 USA

[3] Univ Washington, Dept Astron, Seattle, WA 98195 USA

来源：

ASTROPHYSICAL JOURNAL | 1998年 / 501卷 / 02期

关键词：

galaxies : ISM; gamma rays : bursts; ISM : bubbles; supernova remnants;

D O I：

10.1086/311468

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Gamma-ray burst (GRB) explosions are powerful and frequent enough to make kiloparsec-size shells and holes in the interstellar media of spiral and irregular galaxies. The observations of such remnants are summarized. Several observed shells contain no obvious central star clusters and could be GRB remnants, but sufficiently old clusters, which could have formed these shells by supernovae and winds, might be hard to detect.

引用

页码：L163 / L165

页数：3

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