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A common behavior in the late X-ray afterglow of energeticGRB-SN systems

Published online by Cambridge University Press:  22 July 2013

L. Izzo
Affiliation:
Sapienza University of Rome, P.le Aldo Moro 5, 00185 Rome, Italy;. e-mail: [email protected] ICRANet, Piazza della Republica 10, 65122 Pescara, Italy
G.B. Pisani
Affiliation:
Erasmus Mundus Joint Doctorate IRAP PhD. Student, Université de Nice Sophia Antipolis, Nice Cedex 2, Grand Château Parc Valrose, France
M. Muccino
Affiliation:
Sapienza University of Rome, P.le Aldo Moro 5, 00185 Rome, Italy;. e-mail: [email protected]
J.A. Rueda
Affiliation:
Sapienza University of Rome, P.le Aldo Moro 5, 00185 Rome, Italy;. e-mail: [email protected] ICRANet, Piazza della Republica 10, 65122 Pescara, Italy
Y. Wang
Affiliation:
Sapienza University of Rome, P.le Aldo Moro 5, 00185 Rome, Italy;. e-mail: [email protected]
C.L. Bianco
Affiliation:
Sapienza University of Rome, P.le Aldo Moro 5, 00185 Rome, Italy;. e-mail: [email protected] ICRANet, Piazza della Republica 10, 65122 Pescara, Italy
A.V. Penacchioni
Affiliation:
Erasmus Mundus Joint Doctorate IRAP PhD. Student, Université de Nice Sophia Antipolis, Nice Cedex 2, Grand Château Parc Valrose, France
R. Ruffini
Affiliation:
Sapienza University of Rome, P.le Aldo Moro 5, 00185 Rome, Italy;. e-mail: [email protected] ICRANet, Piazza della Republica 10, 65122 Pescara, Italy
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Abstract

The possibility to divide GRBs in different subclasses allow to understand better thephysics underlying their emission mechanisms and progenitors. The induced gravitationalcollapse 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 afterglowemission of this subclass of GRBs, pointing to a common physical mechanism of their lateemission, consistent with the IGC picture.

Type
Research Article
Copyright
© EAS, EDP Sciences 2013

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