Multi-Wavelength Afterglows in Gamma-Ray Bursts: Refreshed Shock and Jet Effects
Abstract
We present an analytical approach to calculate the hydrodynamics of the interaction between a relativistic ejecta and a surrounding medium, whose evolution serves as a model for Gamma-Ray Burst afterglows. We investigate the effect of the relevant model parameters on the X-ray, optical and radio fluxes, and the effect of a refreshed shock energy input and anisotropy in the ejecta on the shape of the light curves. We compare our numerical results to observed afterglows and give a quantitative description of the conditions (geometry and physical parameters) in the ejecta that are compatible with the light curves of the 970508 afterglow, for which a large number of accurate flux measurements are available.
Cite
@article{arxiv.astro-ph/9801258,
title = {Multi-Wavelength Afterglows in Gamma-Ray Bursts: Refreshed Shock and Jet Effects},
author = {A. Panaitescu and P. Meszaros and M. J. Rees},
journal= {arXiv preprint arXiv:astro-ph/9801258},
year = {2009}
}
Comments
14 pages, 3 figures, to appear in ApJ, vol. 503; revised version, errors in some equations corrected, Figure 1 altered (includes a new parameter: the electron injection fraction), the discussion of the inhomogeneous external medium case (section [4]) was extended, references up-dated