On the "canonical behaviour" of the X-ray afterglows of the Gamma Ray Bursts observed with Swift's XRT

Details On the "canonical behaviour" of the X-ray afterglows of the Gamma Ray Bursts observed with Swift's XRT On the "canonical behaviour" of the X-ray afterglows of the Gamma Ray Bursts observed with Swift's XRT

2005-12-07

arxiv.org/abs/astro-ph/0512196v3

Astrophys.J.646:L21-L24,2006

Astronomy and Astrophysics

Astrophysics

Accepted for publication in ApJL

Scientific paper

10.1086/506606

The "canonical behaviour" of the early X-ray afterglows of long-duration
Gamma-Ray Bursts (GRBs) --observed by the X-Ray Telescope of the SWIFT
satellite-- is precisely the one predicted by the Cannonball model of GRBs.

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