Reverse Shock Emission in Gamma-Ray Bursts Revisited

被引：13

作者：

Gao, He ^{[1
]}

Meszaros, Peter ^{[1
]}

机构：

[1] Penn State Univ, Dept Astron & Astrophys, Ctr Particle & Gravitat Astrophys, Dept Phys,Inst Gravitat & Cosmos, University Pk, PA 16802 USA

来源：

ADVANCES IN ASTRONOMY | 2015年 / 2015卷

关键词：

AFTERGLOW LIGHT CURVES; SWIFT XRT DATA; EARLY OPTICAL AFTERGLOWS; X-RAY; COMPREHENSIVE ANALYSIS; PROMPT EMISSION; GRB; 990123; PHYSICAL PARAMETERS; BLAST WAVES; PANCHROMATIC OBSERVATIONS;

D O I：

10.1155/2015/192383

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A generic synchrotron external shock model is the widely preferred paradigm used to interpret the broadband afterglow data of gamma-ray bursts (GRBs), including predicted observable signatures from a reverse shock which have been confirmed by observations. Investigations of the nature of the reverse shock emission can provide valuable insights into the intrinsic properties of the GRB ejecta. Here we briefly review the standard and the extended models of the reverse shock emission, discussing the connection between the theory and observations, including the implications of the latest observational advances.

引用

页数：16

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