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

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 beh...

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Published inEAS Publications Series Vol. 61; pp. 595 - 597
Main Authors Izzo, L., Pisani, G.B., Muccino, M., Rueda, J.A., Wang, Y., Bianco, C.L., Penacchioni, A.V., Ruffini, R.
Format Journal Article
LanguageEnglish
Published Les Ulis EDP Sciences 2013
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Summary: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.
Bibliography:istex:983DA143B674691887175719309CC9B963064283
publisher-ID:eas1361095
ark:/67375/80W-64VMSLX2-N
PII:S1633476061000957
other:2013EAS....61..595I
e-mail: luca.izzo@gmail.com
ISBN:9782759810024
275981002X
ISSN:1633-4760
1638-1963
DOI:10.1051/eas/1361095