Starling 2007 通过余辉定参数p和k

主要内容:
类似于Panaitescu，对暴进行批量分析。主要是BeppoSAX的暴。

精彩摘抄:


文章信息:
Gamma-Ray Burst Afterglows as Probes of Environment and Blastwave Physics II: the Distribution of p and Structure of the Circumburst Medium

Authors: R. L. C. Starling (1,2), A. J. van der Horst (2), E. Rol (1), R. A. M. J. Wijers (2), C. Kouveliotou (3), K. Wiersema (2), P. A. Curran (2), P. Weltevrede (2) ((1) Leicester, (2) Amsterdam, (3) NASA/MSFC)

(Submitted on 27 Apr 2007)

Abstract: We constrain blastwave parameters and the circumburst media of a subsample of BeppoSAX Gamma-Ray Bursts. For this sample we derive the values of the injected electron energy distribution index, p, and the density structure index of the circumburst medium, k, from simultaneous spectral fits to their X-ray, optical and nIR afterglow data. The spectral fits have been done in count space and include the effects of metallicity, and are compared with the previously reported optical and X-ray temporal behaviour. Assuming the fireball model, we can find a mean value of p for the sample as a whole of 2.04 +0.02/-0.03. A statistical analysis of the distribution demonstrates that the p values in this sample are inconsistent with a single universal value for p at the 3-sigma level or greater, which has significant implications for particle acceleration models. This approach provides us with a measured distribution of circumburst density structures rather than considering only the cases of k=0 (homogeneous) and k=2 (wind-like). We find five GRBs for which k can be well constrained, and in four of these cases the circumburst medium is clearly wind-like. The fifth source has a value of 0 \less k \less 1,>

Comments:

22 pages (single column), 2 figures, submitted to ApJ

Subjects:

Astrophysics (astro-ph)

Cite as:

arXiv:0704.3718v1 [astro-ph]