NDLI: Decay properties of the X-ray afterglows of Gamma-ray bursts

Content Provider	Semantic Scholar
Author	Gendre, Bruce Boer, Michel
Copyright Year	2004
Abstract	We present a set of seventeen Gamma-Ray Bursts (GRBs) with kn own redshifts and X-ray afterglow emission. We apply cosmological corrections in order to compare their flu xes normalized at a redshift of 1. Two classes of GRB can be defi ned using their X-ray afterglow light curves. We show that the br ightest afterglows seem to decay faster than the dimer ones. W also point out evidences for a possible flux limit of the X-ray afterglow depending on the time elapsed since the burst. We t ry to interpret these observations in the framework of the cano nical fireball model of GRB afterglow emission.
File Format	PDF HTM / HTML
Alternate Webpage(s)	http://cds.cern.ch/record/802919/files/0411238.pdf
Alternate Webpage(s)	http://arxiv.org/pdf/astro-ph/0411238v1.pdf
Language	English
Access Restriction	Open
Subject Keyword	Bromides Class Cluster analysis Diagnostic radiologic examination Domino tiling Enigma machine European Union Flux GZMB wt Allele Halobacterium sp. GRB Interferon Type II Newton Redshift Syncope (medicine) Web page X-Ray (Amazon Kindle) Xerox Escape Sequence ginsenoside Rb1 statistical cluster
Content Type	Text
Resource Type	Article

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