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Conference Paper: Physical properties of rapidly decaying Afterglows

TitlePhysical properties of rapidly decaying Afterglows
Authors
Issue Date2013
Citation
Eas Publications Series, 2013, v. 61, p. 217-221 How to Cite?
AbstractWe analyze a sample of Swift X-ray and optical GRB afterglows which were chosen so as to reduce selection effects against the weakest events. We tentatively identify important differences in GRBs that show a fast decay with respect to the average GRB, in particular a tendency for the more energetic bursts to have a steeper afterglow decline. An explanation to this finding could be bursts in a wind environment are on average more energetic than bursts occurring in a constant density medium. © EAS, EDP Sciences 2013.
Persistent Identifierhttp://hdl.handle.net/10722/361257
ISSN
2020 SCImago Journal Rankings: 0.199

 

DC FieldValueLanguage
dc.contributor.authorDe Pasquale, M.-
dc.contributor.authorSchulze, S.-
dc.contributor.authorKann, D. A.-
dc.contributor.authorOates, S.-
dc.contributor.authorZhang, B.-
dc.date.accessioned2025-09-16T04:15:39Z-
dc.date.available2025-09-16T04:15:39Z-
dc.date.issued2013-
dc.identifier.citationEas Publications Series, 2013, v. 61, p. 217-221-
dc.identifier.issn1633-4760-
dc.identifier.urihttp://hdl.handle.net/10722/361257-
dc.description.abstractWe analyze a sample of Swift X-ray and optical GRB afterglows which were chosen so as to reduce selection effects against the weakest events. We tentatively identify important differences in GRBs that show a fast decay with respect to the average GRB, in particular a tendency for the more energetic bursts to have a steeper afterglow decline. An explanation to this finding could be bursts in a wind environment are on average more energetic than bursts occurring in a constant density medium. © EAS, EDP Sciences 2013.-
dc.languageeng-
dc.relation.ispartofEas Publications Series-
dc.titlePhysical properties of rapidly decaying Afterglows-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1051/eas/1361032-
dc.identifier.scopuseid_2-s2.0-84887043257-
dc.identifier.volume61-
dc.identifier.spage217-
dc.identifier.epage221-
dc.identifier.eissn1638-1963-

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