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Conference Paper: Energy injection in GRB afterglows: The case of Swift GRBs 050401, 050801 and 050802

TitleEnergy injection in GRB afterglows: The case of Swift GRBs 050401, 050801 and 050802
Authors
De Pasquale, M.Oates, S.Beardmore, A.Page, K.Blustin, A.Zane, S.Page, M.O'Mason, K.Burrows, D.Palmer, D.Gehrels, N.Nousek, J.Roming, P.Price, P.Zhang, B.Barthelmy, S.Boyd, P.Fink, R.Kobayashi, S.McNought, R.Peterson, B.Rich, J.Rosen, S.Sakamoto, T.Schmidt, B.Tueller, J.Wells, A.Ziaeepour, H.McGowan, K.Poole, X. T.Falcone, A.Blustin, A.
Issue Date2006
Citation
Nuovo Cimento Della Societa Italiana Di Fisica B, 2006, v. 121, n. 12, p. 1471-1473 How to Cite?
DOI: http://dx.doi.org/10.1393/ncb/i2007-10292-y
AbstractSwift unprecedented fast follow-up observations of gamma-ray bursts have allowed us to discover a new feature of GRB afterglows: a phase of shallow decay, usually attributed to energy injection in the burst ejecta, which can last for several thousands of seconds both in the X-ray and optical bands. Here I discuss this phase in the case of Swift GRBs 050401, 050801 and 050802. © Società ltaliana di Fisica.
Persistent Identifierhttp://hdl.handle.net/10722/361096
ISSN
1594-9982

 

DC FieldValueLanguage
dc.contributor.authorDe Pasquale, M.-
dc.contributor.authorOates, S.-
dc.contributor.authorBeardmore, A.-
dc.contributor.authorPage, K.-
dc.contributor.authorBlustin, A.-
dc.contributor.authorZane, S.-
dc.contributor.authorPage, M.-
dc.contributor.authorO'Mason, K.-
dc.contributor.authorBurrows, D.-
dc.contributor.authorPalmer, D.-
dc.contributor.authorGehrels, N.-
dc.contributor.authorNousek, J.-
dc.contributor.authorRoming, P.-
dc.contributor.authorPrice, P.-
dc.contributor.authorZhang, B.-
dc.contributor.authorBarthelmy, S.-
dc.contributor.authorBoyd, P.-
dc.contributor.authorFink, R.-
dc.contributor.authorKobayashi, S.-
dc.contributor.authorMcNought, R.-
dc.contributor.authorPeterson, B.-
dc.contributor.authorRich, J.-
dc.contributor.authorRosen, S.-
dc.contributor.authorSakamoto, T.-
dc.contributor.authorSchmidt, B.-
dc.contributor.authorTueller, J.-
dc.contributor.authorWells, A.-
dc.contributor.authorZiaeepour, H.-
dc.contributor.authorMcGowan, K.-
dc.contributor.authorPoole, X. T.-
dc.contributor.authorFalcone, A.-
dc.contributor.authorBlustin, A.-
dc.date.accessioned2025-09-16T04:14:42Z-
dc.date.available2025-09-16T04:14:42Z-
dc.date.issued2006-
dc.identifier.citationNuovo Cimento Della Societa Italiana Di Fisica B, 2006, v. 121, n. 12, p. 1471-1473-
dc.identifier.issn1594-9982-
dc.identifier.urihttp://hdl.handle.net/10722/361096-
dc.description.abstractSwift unprecedented fast follow-up observations of gamma-ray bursts have allowed us to discover a new feature of GRB afterglows: a phase of shallow decay, usually attributed to energy injection in the burst ejecta, which can last for several thousands of seconds both in the X-ray and optical bands. Here I discuss this phase in the case of Swift GRBs 050401, 050801 and 050802. © Società ltaliana di Fisica.-
dc.languageeng-
dc.relation.ispartofNuovo Cimento Della Societa Italiana Di Fisica B-
dc.titleEnergy injection in GRB afterglows: The case of Swift GRBs 050401, 050801 and 050802-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1393/ncb/i2007-10292-y-
dc.identifier.scopuseid_2-s2.0-35348944855-
dc.identifier.volume121-
dc.identifier.issue12-
dc.identifier.spage1471-
dc.identifier.epage1473-

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