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Modelling of Galaxy Evolution and Interstellar Medium

We are the Chemodynamics Group at the Department of Astrophysics at the University of Vienna. We numerically investigate different aspects of the Interstellar Medium (ISM) by means of the adaptive-mesh refinement code FLASH. Furthermore, we track the chemical evolution of galaxies using a single-gas chemo-dynamical SPH/N-body code.


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Department of Astrophysics
University of Vienna
Türkenschanzstraße 17
1180 Wien
T: +43-1-4277-51895
F: +43-1-4277-9518
University of Vienna | Universitätsring 1 | 1010 Vienna | T +43-1-4277-0
Lastupdate: 14.02.2013 - 22:29