activity
20012004
most citedSimulations of unstable gaseous disks and the origin of giant planets

5 citations · 11 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph2004

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…

astro-ph20042 cited

Cosmological particle-based simulations of galaxy formation; numerical loss of angular momentum and disk heating

Lucio Mayer

We discuss the role that numerical effects have in cosmological N-Body/SPH simulations of disk galaxy formation. We show that the resolution of current state-of-the-art calculation…

astro-ph2003

On the formation of the Magellanic Stream

C. Mastropietro, B. Moore, L. Mayer +2

We use high resolution N-Body/SPH simulations to study the hydro-dynamical and gravitational interaction between the Large Magellanic Cloud and the Milky Way. We model the dark and…

astro-ph2003

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…

astro-ph20034 cited

Galaxies and Overmerging: What Does it Take to Destroy a Satellite Galaxy?

Stelios Kazantzidis, Ben Moore, Lucio Mayer

The Ultra Compact Dwarf (UCD) galaxies recently discovered in the Fornax and Virgo clusters exhibit structural similarity to the dense nuclei of nucleated dEs indicating that the p…

astro-ph20035 cited

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…