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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 ,
G.B. Pisani ,
M. Muccino ,
J.A. Rueda ,
Y. Wang ,
C.L. Bianco ,
A.V. Penacchioni  and
R. Ruffini
L. Izzo
Affiliation:
Sapienza University of Rome, P.le Aldo Moro 5, 00185 Rome, Italy;. e-mail: luca.izzo@gmail.com 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: luca.izzo@gmail.com
J.A. Rueda
Affiliation:
Sapienza University of Rome, P.le Aldo Moro 5, 00185 Rome, Italy;. e-mail: luca.izzo@gmail.com 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: luca.izzo@gmail.com
C.L. Bianco
Affiliation:
Sapienza University of Rome, P.le Aldo Moro 5, 00185 Rome, Italy;. e-mail: luca.izzo@gmail.com 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: luca.izzo@gmail.com 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
Information
European Astronomical Society Publications Series , Volume 61: Gamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe , 2013 , pp. 595 - 597
Copyright
© EAS, EDP Sciences 2013

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References

Arnett, W.D., & Meakin, C., 2011, ApJ, 733, 78 CrossRef
Bernardini, M.G., Margutti, R., Mao, J., et al., 2012, A&A, 539, A3
Cano, Z., Bersier, D., Guidorzi, C., et al., 2011, MNRAS, 413, 669 CrossRef
D’Agostini, G., 2005 [arXiv:physics/0511182]
D’Avanzo, P., Melandri, A., Palazzi, E., et al., 2012, GCN 13609
Dainotti, M.G., Willingale, R., Capozziello, S., et al., 2010, ApJ, 722, 215 CrossRef
Izzo, L., Rueda, J.A., & Ruffini, R., 2012, A&A, 548, L5
Izzo, L., Penacchioni, A.V., Ruffini, R., et al., 2012, A&A, 543, A10
Kann, A., Schulze, S., & Updike, A.C., 2008, GCN 7627
Larsson, J., Ryde, F., Lundman, C., et al., 2011, MNRAS, 414, 2642 CrossRef
Negreiros, R., Rueda, J.A., Bianco, C.L., et al., 2012, A&A, 540, A12
Penacchioni, A.V., Ruffini, R., Izzo, L., et al., 2012, A&A, 538, A58
Penacchioni A.V., Ruffini, R., Bianco, C.L., et al., 2013 [arXiv:1301.6014]
Rueda, J.A., & Ruffini, R., 2012, ApJ, 758, L7 CrossRef
Ruffini, R., Bianco, C.L., Fraschetti, F., et al., 2001, ApJ, 555, L117 CrossRef
Ruffini, R., Bernardini, M.G., Bianco, C.L., et al., 2007, ESA Sp. Pub., 622, 561