Ponente
Descripción
Relativistic jets interact with multiple obstacles as they cross their host galaxies, before interacting with the interstellar or intergalactic medium at hotspots, in powerful sources, or plumes, in low power ones. We assume the possibility that a supernova explosion happens within the jet, and this may have a strong impact not only on the jet dynamics during the evolution of the supernova remnant, but also in terms of radiative output via acceleration at the shock region. We expect the particles acceleration to be enough to reach detectable emissions up to gamma rays.
In this contribution, we present relativistic hydrodynamics simulations of a supernova explosion within an extragalactic jet, with a focus on the dynamics of the interaction and the theoretical radiative output of such events.
