伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章,另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.

星期一, 七月 09, 2007

Genet 2007 对GRB 050820a的拟合

主要内容:
此暴有早期的光学余辉。作者用类似于内激波+正反激波的模型解释暴本身和早期的光学余辉。

精彩摘抄:


文章信息:
arXiv:0707.0952 [ps, pdf, other]

Title: The rise of the afterglow in GRB 050820a
Comments: 6 pages, 9 figures, accepted for publication in A&A
Subjects: Astrophysics (astro-ph)
The early optical afterglow of GRB 050820a recorded by the RAPTOR telescope shows both a contribution from the prompt emission and the initial rise of the afterglow. It is therefore well-suited for the study of the dynamical evolution of the GRB ejecta when it first undergoes the decelerating effect of the environment. This is a complex phase where the internal, reverse, and forward shocks can all be present simultaneously. We have developed a simplified model that can follow these different shocks in an approximate, but self-consistent way. It is applied to the case of GRB 050820a to obtain the prompt and afterglow light curves. We show that the rise of the afterglow during the course of the prompt emission has some important consequences. The reverse shock propagates back into the ejecta before internal shocks are completed, which affects the shape of the gamma-ray profile. We get the best results when the external medium has a uniform density, but obtaining a simultaneous fit of the prompt and afterglow emission is not easy. We discuss a few possibilities that could help to improve this situation

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