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arXiv · 0709.0636

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

Gerhard Hensler·Simone Recchi·Danica Kroeger·Tim Freyer
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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.

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Gerhard Hensler, Simone Recchi, Danica Kroeger, Tim Freyer. 2007-09-05. Internal chemo-dynamical Modeling of Gas Exchange within Galaxies and with their Environment. https://arxiv.org/abs/0709.0636

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