Internal chemo-dynamical Modeling of Gas Exchange within Galaxies and with their Environment

Abstract

By a few but important examples as models of combined radiative and wind-driven Hii regions and galactic winds we demonstrate the importance of refined small-to-medium scale studies of chemo-dynamical effects. These processes determine the internal dynamics and energetic of the ISM and affect its observational signatures, e.g. by abundance contributions, but are not yet reliably and satisfactorily explored.