Theoretical and Numerical Astrophysics
|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.
|Modelling of Photon Dominated Regions|
|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.
|Stellar population synthesis in unresolved galaxies|