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