Internal chemo-dynamical Modeling of Gas Exchange within Galaxies and with their Environment
arXiv:0709.0636
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.
8 pages, 3 fig.s, to be published in conference proceed. ''Pathways through an eclectic Universe'', ASP Conference Series, 2007, J. H. Knapen, T. J. Mahoney, and A. Vazdekis (Eds.)