Building Planets with Dusty Gas
Sarah Maddison, Robin Humble & James Murray
We present animations from 6 simulations which show the effects that
grain size has on the disk morphology of an initially prolate spheroid of
rotating, self-gravitating dusty gas (with a star at the centre) that spins
down to near-equilibrium. The simulations have 12.5K gas + 12.5K dust models
of various grain sizes and are followed for approximately 104
years. The "high resolution" case for 1mm sized grains has 125K gas + 125 K
dust particles. For full simulation parameters, see the
Maddison, Humble &
Murray paper.