Zurich 17-21 September 2007
Next generation of computational models of baryonic physics in galaxy formation: from protostellar cores to disk galaxies Organizers: Francesco Miniati Lucio Mayer Elena D’Onghia
Topics
Formation of molecular clouds
Efficiency of star formation in molecular clouds
Feedback processes in the interstellar medium
Star formation in disk galaxies
Sub-grid models of star formation and feedback in disk galaxy formation
Collapse and cooling of baryons in galaxy-sized dark halos
The angular momentum problem in cosmological disk galaxy formation