Physical Difference between the short and long GRBs

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dc.creatorBalazs, L. G.
dc.creatorBagoly, Z.
dc.creatorHorvath, I.
dc.creatorMeszaros, A.
dc.creatorMeszaros, P.
dc.date2007-02-06
dc.date.accessioned2026-07-07T07:46:05Z
dc.date.available2026-07-07T07:46:05Z
dc.descriptionWe provided separate bivariate log-normal distribution fits to the BATSE short and long burst samples using the durations and fluences. We show that these fits present an evidence for a power-law dependence between the fluence and the duration, with a statistically significant different index for the long and short groups. We argue that the effect is probably real, and the two subgroups are different physical phenomena. This may provide a potentially useful constraint for models of long and short bursts.
dc.description2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0702152
dc.identifierhttp://arxiv.org/abs/astro-ph/0702152
dc.identifierBaltic Astron. 12 (2004) 207-210
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/123713
dc.subjectAstrophysics
dc.titlePhysical Difference between the short and long GRBs
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