Theoretical and Numerical Astrophysics
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Dynamical Studies of Astrophysical Disks: Different numerical methods are used to simulate the gas and stellar dynamics of protoplanetary discs around young stars in cluster environments. |
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Modelling of Photon Dominated Regions |
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Comparing turbulent structures in models and observations: The structure of molecular clouds is complex, often filamentary. Measuring this structure and comparing observations with models will help to understand the nature of interstellar turbulence. |
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Stellar population synthesis in unresolved galaxies |