We work on different aspects of star formation in the Galaxy as well as in the
early universe. We study interstellar turbulence and formation and evolution of
molecular clouds. We are also interested in the dynamical evolution of the
Milky Way and its satellite galaxies. As our work relies heavily on computer
simulations, we also work on developing and improving numerical methods for
Current Research Highlights:
Snapshots of four hydrodynamic simulations of the ISM in starbursting galaxies.
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