328 citations · 3.2k across the 75 of their papers we have counts for
5 papers · 2 filters
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…
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…
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…
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…