Are X-ray flashes a peculiar class of (soft) gamma-ray bursts ?

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dc.creatorDaigne, Frederic
dc.creatorBarraud, Celine
dc.creatorMochkovitch, Robert
dc.date2002-12-02
dc.date.accessioned2026-07-07T02:06:39Z
dc.date.available2026-07-07T02:06:39Z
dc.descriptionHeise et al. (2001) have reported the identification of a new class of sources by Beppo-SAX, the so-called X-ray flashes (XRFs), which have many common properties with gamma-ray bursts (GRBs) but are not detected in the gamma-ray range. In the framework of the internal shock model, we investigate the possibility that XRFs have the same origin than GRBs but are intrinsically softer due to different shock parameters.
dc.description2 pages. To appear in SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0212025
dc.identifierhttp://arxiv.org/abs/astro-ph/0212025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5438
dc.subjectAstrophysics
dc.titleAre X-ray flashes a peculiar class of (soft) gamma-ray bursts ?
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