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dc.contributor.authorCurran, Peter
dc.contributor.authorStarling, R.
dc.contributor.authorO’Brien, P.
dc.contributor.authorGodet, O.
dc.contributor.authorvan der Horst, A.
dc.contributor.authorWijers, R.
dc.identifier.citationCurran, P. and Starling, R. and O’Brien, P. and Godet, O. and van der Horst, A. and Wijers, R. 2008. On the nature of late X-ray flares in Swift gamma-ray bursts. Astronomy and Astrophysics. 487: pp. 533-538.

Context. Previously detected in only a few gamma-ray bursts (GRBs), X-ray flares are now observed in ~50% of Swift GRBs, thoughtheir origins remain unclear. Most flares are seen early on in the afterglow decay, while some bursts exhibit flares at late times of 104to 105 s, which may have implications for flare models.Aims. We investigate whether a sample of late time (1 × 104 s) flares are different from previous samples of early time flares, orwhether they are merely examples on the tail of the early flare distribution.Methods. We examine the X-ray light curves of Swift bursts for late flares and compare the flare and underlying temporal power-lawproperties with those of early flares, and the values of these properties predicted by the blast wave model.Results. The burst sample shows late flare properties consistent with those of early flares, where the majority of the flares can beexplained by either internal or external shock, though in a few cases one origin is favoured over the other. The underlying power-lawsare mainly consistent with the normal decay phases of the afterglow.Conclusions. If confirmed by the ever growing sample of late time flares, this would imply that, in some cases, prolonged activity outto a day or a restarting of the central engine is required.

dc.publisherEDP Sciences
dc.subjectradiation mechanisms: non-thermal
dc.subjectX-rays: bursts
dc.subjectgamma rays: bursts
dc.titleOn the nature of late X-ray flares in Swift gamma-ray bursts
dc.typeJournal Article
dcterms.source.titleAstronomy and Astrophysics
curtin.accessStatusFulltext not available

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