On the nature of X-ray Flashes

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dc.creatorMochkovitch, Robert
dc.creatorDaigne, Frederic
dc.creatorBarraud, Celine
dc.creatorAtteia, Jean-Luc
dc.date2003-03-13
dc.date.accessioned2026-07-07T02:07:54Z
dc.date.available2026-07-07T02:07:54Z
dc.descriptionWe have developed a toy model for internal shocks which has been used to generate a large number of synthetic GRBs in order to find in the parameter space the conditions which can lead to the formation of X-ray flashes. The key condition appears to be a small contrast of the Lorentz factor in the relativistic wind emitted by the central engine.
dc.description4 pages, 4 figures, to appear in "Gamma-ray bursts in the afterglow era", 3rd workshop, Rome 17-20 Sept. 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0303289
dc.identifierhttp://arxiv.org/abs/astro-ph/0303289
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5852
dc.subjectAstrophysics
dc.titleOn the nature of X-ray Flashes
dc.typetext

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