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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…
A universal density slope - velocity anisotropy relation for relaxed structures
Steen H. Hansen, Ben Moore
We identify a universal relation between the radial density slope α(r) and the velocity anisotropy β(r) for equilibrated structures. This relation holds for a variety of systems, i…
Bulges or Bars from Secular Evolution?
Victor P. Debattista, C. Marcella Carollo, Lucio Mayer +1
We use high resolution collisionless -body simulations to study the secular evolution of disk galaxies and in particular the final properties of disks that suffer a bar and perh…
Convergence and scatter of cluster density profiles
Juerg Diemand, Ben Moore, Joachim Stadel
We present new results from a series of LCDM simulations of cluster mass halos resolved with high force and mass resolution. These results are compared with recently published simu…
Velocity and spatial biases in CDM subhalo distributions
Juerg Diemand, Ben Moore, Joachim Stadel
We present a statistical study of substructure within a sample of LCDM clusters and galaxies simulated with up to 25 million particles. With thousands of subhalos per object we can…