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dc.contributor.authorCurran, Peter
dc.contributor.authorKann, D.
dc.contributor.authorFerrero, P.
dc.contributor.authorRol, E.
dc.date.accessioned2017-01-30T15:16:29Z
dc.date.available2017-01-30T15:16:29Z
dc.date.created2015-09-29T02:03:57Z
dc.date.issued2006
dc.identifier.citationCurran, P. and Kann, D. and Ferrero, P. and Rol, E. 2006. The prompt emission & peculiar break of GRB060124. Il Nuovo Cimento B. 2006 (12): pp. 1461-1462.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/44793
dc.identifier.doi10.1393/ncb/i2007-10278-9
dc.description.abstract

Our multi-wavelength analysis of GRB060124 shows the unusual behaviour of the decaying lightcurve as well as supporting the recently proposed phenomenon of long- lasting central engine activity. The prompt X-ray emission displays uncommonly well resolved flaring behaviour, with spectral evolution – indicative of central engine activity – which allows us to estimate the energy injection time for each flare. The otherwise smooth X-ray & optical afterglows demonstrate achromatic breaks at about 1 day which differ significantly from the usual jet break in the blastwave model of afterglows.

dc.publisherSocieta Italiana di Fisica (S I F)
dc.relation.urihttp://arxiv.org/pdf/astro-ph/0610067v2.pdf
dc.titleThe prompt emission & peculiar break of GRB060124
dc.typeJournal Article
dcterms.source.volume2006
dcterms.source.number12
dcterms.source.startPage1461
dcterms.source.endPage1462
dcterms.source.issn2037-4895
dcterms.source.titleIl Nuovo Cimento B
curtin.accessStatusFulltext not available


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