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A common behavior in the late X-ray afterglow of energetic GRB-SN systems
Published online by Cambridge University Press: 22 July 2013
Abstract
The possibility to divide GRBs in different subclasses allow to understand better the physics underlying their emission mechanisms and progenitors. The induced gravitational collapse scenario proposes a binary progenitor to explain the time-sequence in GRBs-SNe. We show the existence of a common behavior of the late decay of the X-ray afterglow emission of this subclass of GRBs, pointing to a common physical mechanism of their late emission, consistent with the IGC picture.
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- Research Article
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- © EAS, EDP Sciences 2013
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