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The evolution of gravitationally unstable protoplanetary disks: fragmentation and possible giant planet formation
Lucio Mayer, Thomas Quinn, James Wadsley +1
We carry out a large set of very high resolution, three dimensional smoothed particle hydrodynamics (SPH) simulations describing the evolution of gravitationally unstable gaseous p…
Sweeping and shaking dwarf satellites
Lucio Mayer, James Wadsley
We present the first high-resolution N-Body/SPH simulations that follow the evolution of low surface brightness disk satellites in a primary halo containing both dark matter and a…
Simulations of Gaseous Disc-Embedded Planet Interaction
Graeme Lufkin, Thomas Quinn, James Wadsley +2
We present three-dimensional self-gravitating smoothed-particle hydrodynamics (SPH) simulations of an isothermal gaseous disc interacting with an embedded planet. Discs of varying…
Gasoline: An adaptable implementation of TreeSPH
James Wadsley, Joachim Stadel, Thomas Quinn
The key algorithms and features of the Gasoline code for parallel hydrodynamics with self-gravity are described. Gasoline is an extension of the efficient Pkdgrav parallel N-body c…
The formation and evolution of bars in low surface brightness galaxies with cold dark matter halos
Lucio Mayer, James Wadsley
We perform several high resolution N-Body/SPH simulations of low surface brightness galaxies (LSBs) embedded in cold dark matter halos to study how likely is bar formation in such…
Simulations of unstable gaseous disks and the origin of giant planets
Lucio Mayer, Thomas Quinn, James Wadsley +1
We study the evolution of cold, gravitationally unstable protoplanetary gaseous disks performing 3D SPH simulations with up to a million particles on large parallel machines. We sh…