Objetivo The physical conditions in relativistic jets generated in vicinity of black holes or neutron stars may not be directly accessible to current observations, the reason being that the detected radiation originates from a non-thermal population of relativistic particles which may represent only a part of a more complex system (including a thermal component carying most of the mass of a jet). This project applies state-of-the-art numerical techniques as well as carefully developed analytic models to link the phy sical state of the jet to the radiation associated with the gamma ray bursts (GRBs) and active galactic nuclei (AGN). Ámbito científico natural sciencesphysical sciencesastronomystellar astronomyneutron starsnatural sciencesphysical sciencesastronomyastrophysicsblack holesnatural sciencesphysical sciencesastronomyobservational astronomyx-ray astronomynatural sciencesphysical sciencesastronomyplanetary sciencescelestial mechanicsengineering and technologyelectrical engineering, electronic engineering, information engineeringelectronic engineeringcomputer hardwaresupercomputers Palabras clave non-thermal radiation processes numerical hydrodynamics Programa(s) FP6-MOBILITY - Human resources and Mobility in the specific programme for research, technological development and demonstration "Structuring the European Research Area" under the Sixth Framework Programme 2002-2006 Tema(s) MOBILITY-2.3 - Marie Curie Incoming International Fellowships (IIF) Convocatoria de propuestas FP6-2004-MOBILITY-7 Consulte otros proyectos de esta convocatoria Régimen de financiación EIF - Marie Curie actions-Intra-European Fellowships Coordinador UNIVERSITAT DE VALÈNCIA. ESTUDI GENERAL Aportación de la UE Sin datos Dirección Avda. Blasco Ibañez, 13. VALENCIA España Ver en el mapa Enlaces Sitio web Opens in new window Coste total Sin datos