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

2); (2) INAF - Osservatorio Astronomico di Trieste; (3) Institute of Theor. Physics & Astrophysics; Danica Kroeger (3); Gerhard Hensler (1); Simone Recchi (1; Tim Freyer (3) ((1) Institute of Astronomy; University of Kiel); University of Vienna

arxiv: 0709.0636 · v1 · submitted 2007-09-05 · 🌌 astro-ph

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

Gerhard Hensler (1) , Simone Recchi (1 , 2) , Danica Kroeger (3) , Tim Freyer (3) ((1) Institute of Astronomy , University of Vienna , (2) INAF - Osservatorio Astronomico di Trieste , (3) Institute of Theor. Physics & Astrophysics

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University of Kiel)

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keywords chemo-dynamicalinternalabundanceaffectcombinedcontributionsdemonstratedetermine

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

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