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astro-ph2007128 cited

Simulating the Bullet Cluster

Chiara Mastropietro, Andreas Burkert

We present high resolution N-body/SPH simulations of the interacting cluster 1E0657-56. The main and the sub-cluster are modeled using extended cuspy LCDM dark matter halos and iso…

astro-ph2005

Simultaneous ram pressure and tidal stripping; how dwarf spheroidals lost their gas

Lucio Mayer, Chiara Mastropietro, James Wadsley +2

We perform high-resolution N-Body+SPH simulations of gas-rich dwarf galaxy satellites orbiting within a Milky Way-sized halo and study for the first time the combined effects of ti…

astro-ph2004

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…

astro-ph2004

Morphological evolution of disk galaxies in clusters

Chiara Mastropietro, Ben Moore, Lucio Mayer +3

The recent discovery of hidden non-axysimmetric and disk-like structures in bright Virgo dwarf elliptical and lenticular galaxies (dE/dSph/dS0) indicates that they may have late-ty…

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…