XRT Light curves: Morphology, Flares and Energy

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dc.creatorChincarini, G.
dc.creatorMangano, V.
dc.creatorMoretti, A.
dc.creatorPerri, M.
dc.creatorRomano, P.
dc.creatorCampana, S.
dc.creatorCovino, S.
dc.creatorTagliaferri, G.
dc.creatorAngelini, L.
dc.creatorBurrows, D.
dc.creatorGiommi, P.
dc.creatorOsborne, J.
dc.creatorTeam, Swift
dc.date2005-11-03
dc.date.accessioned2026-07-07T06:44:52Z
dc.date.available2026-07-07T06:44:52Z
dc.descriptionFollowing a brief introduction we show that the observations obtained so far with the Swift satellite begin to shed light over a variety of problems that were left open following the excellent performance and related discoveries of the Italian - Dutch Beppo SAX satellite. The XRT light curves show common characteristics that are reasonably understood within the framework of the fireball model. Unforeseen flares are however detected in a large fraction of the GRB observed and the energy emitted by the brightest ones may be as much as 85% of the total soft X ray emission measured by XRT. These characteristics seems to be common to long and short bursts.
dc.description6 pages, 9 figures. Proceedings of conference "The X-Ray Universe", San Lorenzo de El Escorial (Madrid, Spain), 26-30 September 2005
dc.identifierhttps://arxiv.org/abs/astro-ph/0511107
dc.identifierhttp://arxiv.org/abs/astro-ph/0511107
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102893
dc.subjectAstrophysics
dc.titleXRT Light curves: Morphology, Flares and Energy
dc.typetext

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