Gamma-ray burst beaming:: A universal configuration with a standard energy reservoir?

被引:287
作者
Zhang, B [1 ]
Mészáros, P [1 ]
机构
[1] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16803 USA
关键词
gamma rays : bursts; ISM : jets and outflows; shock waves;
D O I
10.1086/339981
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a gamma-ray burst (GRB) model based on an anisotropic fireball with an axisymmetric energy distribution of the form epsilon(theta) proportional to theta(-k) and allow for the observer's viewing direction being at an arbitrary angle theta(v) with respect to the jet axis. This model can reproduce the key features expected from the conventional on-axis uniform jet models, with the novelty being that the achromatic break time in the broadband afterglow light curves corresponds to the epoch during which the relativistic beaming angle is equal to the viewing angle, theta(v), rather than to the jet half-opening angle, theta(j). If all the GRB reballs have such a similar energy distribution form with 1.5 < k ≲ 2, then GRBs may be modeled by a quasi-universal beaming configuration and an approximately standard energy reservoir. This conclusion also holds for some other forms of angular energy distributions, such as the Gaussian function.
引用
收藏
页码:876 / 879
页数:4
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