The early high-energy afterglow emission from short GRBs

来源 :中国科学：物理学、力学、天文学英文版 | 被引量 : 0次 | 上传用户：haose1989

【摘要】

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We calculate the high energy afterglow emission from short Gamma-Ray Bursts(SGRBs) in the external shock model.There are two possible components contributing to

【出处】

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中国科学：物理学、力学、天文学英文版

【发表日期】

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2010年S1期

【关键词】

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GAMMA-RAY BURST RADIATION mechanism BLAST wave gamma-ray burstradiation mechanis

【基金项目】

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supported by the National Basic Research Program of China (Grant No. 2009CB824800),the Foundation for the Authors of National Excellent Doctoral Dissertations of China,the Qing Lan Project and the NCE

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We calculate the high energy afterglow emission from short Gamma-Ray Bursts(SGRBs) in the external shock model.There are two possible components contributing to the high energy afterglow:electron synchrotron emission and synchrotron self-Compton(SSC) emis

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The early high-energy afterglow emission from short GRBs

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