High-redshift gamma-ray bursts

被引：0
|
作者：
Chen, Hsiao-Wen [1 ]
Bloom, Josh S. [2 ]
Prochaska, Jason X. [3 ]
机构：
[1] Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA
[2] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[3] Univ Calif Santa Cruz, UCO Lick Observ, Santa Cruz, CA 95064 USA
来源：
FIRST STARS III | 2008年 / 990卷
关键词：
gamma-ray burst; interstellar medium; intergalactic medium; starburst; LYMAN-CONTINUUM EMISSION; COSMIC CHEMICAL EVOLUTION; INTERSTELLAR-MEDIUM; HOST GALAXIES; AFTERGLOW SPECTROSCOPY; BRIGHT SUPERNOVA; ESCAPE FRACTION; LOW METALLICITY; CORE-COLLAPSE; CONSTRAINTS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Gamma-ray bursts (GRBs) mark a grand finale of stellar evolution. GRBs are among the most energetic events in the universe after the Big Bang. Significant progress has been made in the past few years in understanding the nature of the GRB progenitors through rapid imaging and spectroscopic followups. Here we provide a brief review of what we have learned about their properties from early-time light curve studies and afterglow spectroscopy. We also review the utility of GRB afterglows as cosmic probes to study the distant universe.
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收藏
页码：473 / +
页数：4
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