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

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dc.creatorHensler, Gerhard
dc.creatorRecchi, Simone
dc.creatorKroeger, Danica
dc.creatorFreyer, Tim
dc.date2007-09-05
dc.date.accessioned2026-07-07T08:27:44Z
dc.date.available2026-07-07T08:27:44Z
dc.descriptionBy 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.
dc.description8 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.)
dc.identifierhttps://arxiv.org/abs/0709.0636
dc.identifierhttp://arxiv.org/abs/0709.0636
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/137371
dc.subjectAstrophysics
dc.titleInternal chemo-dynamical Modeling of Gas Exchange within Galaxies and with their Environment
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