The prompt emission & peculiar break of GRB060124
dc.contributor.author | Curran, Peter | |
dc.contributor.author | Kann, D. | |
dc.contributor.author | Ferrero, P. | |
dc.contributor.author | Rol, E. | |
dc.date.accessioned | 2017-01-30T15:16:29Z | |
dc.date.available | 2017-01-30T15:16:29Z | |
dc.date.created | 2015-09-29T02:03:57Z | |
dc.date.issued | 2006 | |
dc.identifier.citation | Curran, 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.uri | http://hdl.handle.net/20.500.11937/44793 | |
dc.identifier.doi | 10.1393/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.publisher | Societa Italiana di Fisica (S I F) | |
dc.relation.uri | http://arxiv.org/pdf/astro-ph/0610067v2.pdf | |
dc.title | The prompt emission & peculiar break of GRB060124 | |
dc.type | Journal Article | |
dcterms.source.volume | 2006 | |
dcterms.source.number | 12 | |
dcterms.source.startPage | 1461 | |
dcterms.source.endPage | 1462 | |
dcterms.source.issn | 2037-4895 | |
dcterms.source.title | Il Nuovo Cimento B | |
curtin.accessStatus | Fulltext not available |