Relativistic Outflows in Gamma Ray Bursts

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dc.creatorStern, Boris
dc.date1999-02-15
dc.date.accessioned2026-07-07T02:30:27Z
dc.date.available2026-07-07T02:30:27Z
dc.descriptionDespite that gamma-ray bursts is a phenomenon quite different from accreting compact objects, it could be that their hard X-ray emission is associated with a very similar mechanism of energy dissipation. In both cases, we could deal with reconnection of a turbulent magnetic field with intensive e+e- pair production and quasi-thermal Comptonization.
dc.description15 pages; Invited review at the workshop "High Energy Processes in Accreting Black Holes", eds. J. Poutanen and R. Svensson, ASP Conf. Series, Vol. 161, p. 277
dc.identifierhttps://arxiv.org/abs/astro-ph/9902203
dc.identifierhttp://arxiv.org/abs/astro-ph/9902203
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13823
dc.subjectAstrophysics
dc.titleRelativistic Outflows in Gamma Ray Bursts
dc.typetext

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