Afterglow light curves from magnetized GRB flows

被引:0
作者
Mimica, Petar [1 ]
Giannios, Dimitrios
Aloy, Miguel Angel [1 ]
机构
[1] Univ Valencia, Dept Astron & Astrofis, E-46100 Burjassot, Spain
来源
JETS AT ALL SCALES | 2011年 / 275期
关键词
hydrodynamics (magnetohydrodynamics:) MHD; radiation mechanisms: nonthermal; radiative transfer; shock waves; methods: numerical; gamma rays: bursts; GAMMA-RAY BURST; JETS; DISSIPATION; EMISSION; ENERGY; FIELDS;
D O I
10.1017/S1743921310016406
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using the RMHD code MRGENESIS and the radiative transfer code SPEV we compute multiwavelength afterglow light curves of magnetized ejecta of gamma-ray bursts interacting with a uniform circumburst medium. We are interested in the emission from the reverse shock when ejecta magnetization varies from sigma(0) = 0 to sigma(0) = 1. For typical parameters of the ejecta, the emission from the reverse shock peaks for magnetization sigma(0) similar to 0.01 - 0.1, and is suppressed for higher sigma(0). We fit the early afterglow light curves of ORB 990123 and 090102 and discuss the possible magnetization of the outflows of these bursts. Finally we discuss the amount energy left in the magnetic field which is available for dissipation at later afterglow stages.
引用
收藏
页码:358 / 362
页数:5
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