Gamma-ray burst afterglows

被引:305
作者
van Paradijs, J
Kouveliotou, C
Wijers, RAMJ
机构
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
[2] Univ Alabama, Huntsville, AL 35899 USA
[3] NASA, George C Marshall Space Flight Ctr, Univ Space Res Assoc, Huntsville, AL 35812 USA
[4] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
基金
美国国家航空航天局;
关键词
gamma-ray bursts; compact objects; cosmology; particle acceleration; shocks; supernovae;
D O I
10.1146/annurev.astro.38.1.379
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The discovery of counterparts in X-ray and optical to radio wavelengths has revolutionized the study of gamma -ray bursts, until recently the most enigmatic of astrophysical phenomena. We now know that gamma -ray bursts are the biggest explosions in nature, caused by the ejection of ultrarelativistic matter from a powerful energy source and its subsequent collision with its environment. We have just begun to uncover a connection between supernovae and gamma -ray bursts, and are finally constraining the properties of the ultimate source of gamma -ray burst energy. We review here the observations that have led to this breakthrough in the field; we describe the basic theory of the fireball model and discuss the theoretical understanding that has been gained from interpreting the new wealth of data on gamma -ray bursts.
引用
收藏
页码:379 / +
页数:66
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