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Energetics-spectral correlations versus the BATSE gamma-ray bursts population

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dc.contributor.author Bosnjak, Zeljka Marija en_US
dc.contributor.author Celotti, Annalisa en_US
dc.contributor.author Longo, Francesco en_US
dc.contributor.author Barbiellini, Guido en_US
dc.date.accessioned 2008-02-21T11:39:27Z en_US
dc.date.accessioned 2011-09-07T20:24:01Z
dc.date.available 2008-02-21T11:39:27Z en_US
dc.date.available 2011-09-07T20:24:01Z
dc.date.issued 2008-02-21T11:39:27Z en_US
dc.identifier.citation MNRAS 384 (2008) 599-604 en_US
dc.identifier.uri http://hdl.handle.net/1963/2588 en_US
dc.description.abstract Recently proposed correlations between the energetics of Gamma-Ray Bursts (GRB) and their spectral properties, namely the peak energy of their prompt emission, are found to account for the observed fluence distribution of all `bright' BATSE GRB. Furthermore for an intrinsic GRB peak energy distribution extending toward lower energies with respect to that characterizing bright GRB, such correlations allow to reproduce the fluence distribution of the whole BATSE long GRB population. We discuss the constraints that such analysis imposes on the shape of the peak energy distribution, the opening angle distribution and the tightness of such correlations. en_US
dc.format.extent 223405 bytes en_US
dc.format.mimetype application/pdf en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries arXiv.org;0502185v1 en_US
dc.relation.uri 10.1111/j.1365-2966.2007.12672.x en_US
dc.title Energetics-spectral correlations versus the BATSE gamma-ray bursts population en_US
dc.type Article en_US
dc.contributor.department Astrophysics en_US
dc.contributor.area Physics en_US

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