Simulations of star formation on a range of scales, from parsec to cosmological volumes, utilizing nested hierarchical methods
Simulations of the life cycle and physical properties of star-forming giant molecular clouds utilizing high-resolultion idealized simulations of disk galaxies and mergers
coupled turtlebeach molecular line radiative transfer calculations with starburst galaxy merger hydrodynamic models allow for physical models for submillimeter-wave observations
Coupled 3D radiative transfer with hydrodynamic simulations results in bona fide observable quantities from numerical simulations
We're organizing a conference on dusty galaxies and reionization: Obergurgl 2014. Email me for details.