About: Early UV/Optical Emission of The Type IB SN 2008D

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Attributs	Valeurs
type	work Article
Is Part Of	Gamma-ray Bursts: 15 Years of GRB Afterglows - Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe
Subject	Chapter VIII: Progenitors and Environments
Title	Early UV/Optical Emission of The Type IB SN 2008D
Date	2013-01-01(xsd:dateTime)
has manifestation of work	http://hub.abes.fr/edp/periodical/eas/2013/volume_61/issue_2013/eas1361058/m/print http://hub.abes.fr/edp/periodical/eas/2013/volume_61/issue_2013/eas1361058/m/web
related by	http://hub.abes.fr/edp/periodical/eas/2013/volume_61/issue_2013/eas1361058/authorship/3 http://hub.abes.fr/edp/periodical/eas/2013/volume_61/issue_2013/eas1361058/authorship/4 http://hub.abes.fr/edp/periodical/eas/2013/volume_61/issue_2013/eas1361058/authorship/2 http://hub.abes.fr/edp/periodical/eas/2013/volume_61/issue_2013/eas1361058/authorship/1
Author	Bersten, M.C.
Editor	Park, I.H. Castro-Tirado, A. J. Gorosabel J.
Abstract	We propose an alternative explanation for the post-breakout emission of SN 2008D that cannot be reproduced by the explosion of a normal Wolf-Rayet star. We explored several physical scenarios and proposed that the early emission was enhanced by the presence of 56Ni in the outermost layers of the ejecta in addition to the usual internal distribution. This kind of double-peaked 56Ni distribution could be explained by the formation of jets during the explosion.
article type	research-article
publisher identifier	eas1361058
Date Copyrighted	2013-01-01(xsd:dateTime)
Rights	© EAS, EDP Sciences 2013
Rights Holder	EAS, EDP Sciences
is part of this journal	EAS Publications Series
is primary topic of	http://hub.abes.fr/edp/periodical/eas/2013/volume_61/issue_2013/eas1361058/w/record

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