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abstract: ‘The present study demonstrates that the Gamma-ray and Cherenkov light curves of the prompt GRB 100206A can be consistently explained by reverse shock emission. This discovery of the GRB 100206A afterglow suggests a new direction of GRB study. Future observations, particularly with the Suzaku satellite, are expected to provide a detailed data set that will allow to test and refine the model developed for GRB 100206A.’
author:
– |
V. Bosch-Ramon,$^{1}$ L. M. Paredes,$^{1}$ C. Dar$^{2}$ and E. de Ugarte Postigo$^{2}$\
$^{1}$Departament d’Astronomia i Astrofísica, Universitat de València, C/ Dr. Moliner 50, 46100 Burjassot, València, Spain\
$^{2}$Instituto de Ciencias del Espacio, UNAM, Dr. Morelos 12 – C. P. 04510, México
date: ‘Accepted 2008 November 20. Received 2008 November 20; in original form 2008 October 15.’
title: ‘Reverse-shock emission in the prompt optical afterglow of GRB 100206A’
—
\[firstpage\]
gamma-rays: bursts – ISM: individual (GRB 100206A)
Introduction
============
Observational evidence shows
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