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伽马射线暴。

Gamma-ray bursts.

机构信息

Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.

出版信息

Science. 2012 Aug 24;337(6097):932-6. doi: 10.1126/science.1216793.

Abstract

Gamma-ray bursts (GRBs) are bright flashes of gamma rays coming from the cosmos. They occur roughly once per day, typically last for tens of seconds, and are the most luminous events in the universe. More than three decades after their discovery, and after pioneering advances from space and ground experiments, they still remain mysterious. The launch of the Swift and Fermi satellites in 2004 and 2008 brought in a trove of qualitatively new data. In this Review, we survey the interplay between these recent observations and the theoretical models of the prompt GRB emission and the subsequent afterglow.

摘要

伽马射线暴(GRB)是来自宇宙的伽马射线的明亮闪光。它们每天大约发生一次,通常持续数十秒,是宇宙中最亮的事件。在发现它们三十多年后,通过太空和地面实验的开创性进展,它们仍然很神秘。Swift 和 Fermi 卫星于 2004 年和 2008 年发射,带来了大量全新的数据。在这篇综述中,我们调查了这些最近的观测结果与 prompt GRB 发射和后续余辉的理论模型之间的相互作用。

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