Jet propagation through inhomogeneous media and shock ionization

Abstract In this contribution, we present the first numerical simulations of a relativistic outflow propagating through inner hundreds parsecs its host galaxy, including atomic and ionized hydrogen, cooling effects ionization. Our results are preliminary, but observe efficient shock ionization hydrogen in interstellar clouds. The mean density medium these initial is lower than that expected typical galaxies, which makes times longer thus no recombination observed inside shocked region. velocities achieved by gas agreement with observational results, although wide spectrum values.