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Conference Paper: Swift observations of GRB050712

TitleSwift observations of GRB050712
Authors
Pasquale, M. D.Poole, T.Zane, S.Page, M.Breeveld, A.O'Mason, K.Grupe, D.Burrows, D.Nousek, J.Roming, P.Krimm, H.Gehrels, N.Zhang, B.Kobayashi, S.
KeywordsGamma Ray Bursts
High energy sources
Ultrarelativistic shocks
Issue Date2008
Citation
11th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity Gravitation and Relativistic Field Theories Proc of the Mg11 Meeting on General Relativity, 2008, p. 1947-1949 How to Cite?
AbstractSwift observations of GRB050712 show that the X-ray lightcurve of this burst exhibits flaring activity in the first 500s. We find that the initial flares can be due to "inner engine" activity, where the later flare may be explained in terms of the interaction of the ejecta with the surrounding medium. An optical counterpart was detected in the U and V band of UVOT up to 15000s after the trigger. © 2008 World Scientific Publishing Co. Pte. Ltd.
Persistent Identifierhttp://hdl.handle.net/10722/361271

 

DC FieldValueLanguage
dc.contributor.authorPasquale, M. D.-
dc.contributor.authorPoole, T.-
dc.contributor.authorZane, S.-
dc.contributor.authorPage, M.-
dc.contributor.authorBreeveld, A.-
dc.contributor.authorO'Mason, K.-
dc.contributor.authorGrupe, D.-
dc.contributor.authorBurrows, D.-
dc.contributor.authorNousek, J.-
dc.contributor.authorRoming, P.-
dc.contributor.authorKrimm, H.-
dc.contributor.authorGehrels, N.-
dc.contributor.authorZhang, B.-
dc.contributor.authorKobayashi, S.-
dc.date.accessioned2025-09-16T04:15:45Z-
dc.date.available2025-09-16T04:15:45Z-
dc.date.issued2008-
dc.identifier.citation11th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity Gravitation and Relativistic Field Theories Proc of the Mg11 Meeting on General Relativity, 2008, p. 1947-1949-
dc.identifier.urihttp://hdl.handle.net/10722/361271-
dc.description.abstractSwift observations of GRB050712 show that the X-ray lightcurve of this burst exhibits flaring activity in the first 500s. We find that the initial flares can be due to "inner engine" activity, where the later flare may be explained in terms of the interaction of the ejecta with the surrounding medium. An optical counterpart was detected in the U and V band of UVOT up to 15000s after the trigger. © 2008 World Scientific Publishing Co. Pte. Ltd.-
dc.languageeng-
dc.relation.ispartof11th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity Gravitation and Relativistic Field Theories Proc of the Mg11 Meeting on General Relativity-
dc.subjectGamma Ray Bursts-
dc.subjectHigh energy sources-
dc.subjectUltrarelativistic shocks-
dc.titleSwift observations of GRB050712-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.scopuseid_2-s2.0-84892975130-
dc.identifier.spage1947-
dc.identifier.epage1949-

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