On the "canonical behaviour" of the X-ray afterglows of the Gamma Ray Bursts observed with Swift's XRT
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🌌 astro-ph
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x-rayafterglowsbehaviourburstscanonicalgrbsobservedswift
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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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