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The gravitational and hydrodynamical interaction between the LMC and the Galaxy
Chiara Mastropietro, Ben Moore, Lucio Mayer +2
We use high resolution N-Body/SPH simulations to study the hydrodynamical and gravitational interaction between the Large Magellanic Cloud and the Milky Way. We model the dark and…
High resolution SPH simulations of disk formation in CDM halos; resolution tests
Tobias Kaufmann, Lucio Mayer, Ben Moore +2
We perform N-Body/SPH simulations of disk galaxy formation inside equilibrium spherical and triaxial cuspy dark matter halos. We systematically study the disk properties and morpho…
Fate of Supermassive Black Holes and Evolution of the M(BH)-sigma Relation in Merging Galaxies: The Effect of Gaseous Dissipation
Stelios Kazantzidis, Lucio Mayer, Monica Colpi +6
We analyze the effect of dissipation on the orbital evolution of supermassive black holes (SMBHs) using high-resolution self-consistent gasdynamical simulations of binary equal- an…
Gravitational instability in binary protoplanetary disks; new constraints on giant planet formation
Lucio Mayer, James Wadsley, Thomas Quinn +1
We use high resolution 3D SPH simulations to study the evolution of self-gravitating binary protoplanetary disks. Heating by shocks and cooling are included. We consider different…
The Origin and Properties of Intracluster Stars in a Rich Cluster
Beth Willman, Fabio Governato, James Wadsley +1
We use a multi million particle N-body + SPH simulation to follow the formation of a rich galaxy cluster in a Lambda+CDM cosmology, with the goal of understanding the origin and pr…