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Gamma-Ray Bursts in the Swift Era

查看全文 作  者:Bing [1]Zhang 高影响力作者 机构地区:[1]Department of Physics & Astronomy, University of Nevada, Las Vegas, NV 89154-4002, USA高影响力机构 出  处:《Chinese Journal of Astronomy and Astrophysics》索引2007年第7卷第1期,共50页高影响力期刊 摘  要:Since the successful launch of NASA’s dedicated gamma-ray burst (GRB) mission, Swift, the study of cosmological GRBs has entered a new era. Here I review the rapid obser- vational and theoretical progress in this dynamical research field during the first two-year of the Swift mission, focusing on how observational breakthroughs have revolutionized our un- derstanding of the physical origins of GRBs. Besides summarizing how Swift helps to solve some pre-Swift mysteries, I also list some outstanding problems raised by the Swift obser-vations. An outlook of GRB science in the future, especially in the GLAST era, is briely discussed. 关 键 词:Swift卫星 Γ射线爆 观察数据 研究进展 美国国家航空和宇宙航行局
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