activity
20032014
most citedSimultaneous ram pressure and tidal stripping; how dwarf spheroidals lost their gas

439 citations · 1.7k across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2014★ 75 cited

Modelling CO emission from hydrodynamic simulations of nearby spirals, starbursting mergers, and high-redshift galaxies

F. Bournaud, E. Daddi, A. Weiss +3

We model the intensity of emission lines from the CO molecule, based on hydrodynamic simulations of spirals, mergers, and high-redshift galaxies with very high resolutions (3pc and…

astro-ph.CO2010★ 346 cited

The VMC Survey - I. Strategy and First Data

M. -R. L. Cioni, G. Clementini, L. Girardi +31

The new VISual and Infrared Telescope for Astronomy (VISTA) has started operations. Over its first five years it will be collecting data for six public surveys, one of these is the…

astro-ph.CO2009★ 58 cited

The First Generation of Virgo Cluster Dwarf Elliptical Galaxies?

T. Lisker, J. Janz, G. Hensler +7

In the light of the question whether most early-type dwarf (dE) galaxies in clusters formed through infall and transformation of late-type progenitors, we search for an imprint of…

astro-ph.CO2009★ 36 cited

Effects of ram pressure on the gas distribution and star formation in the Large Magellanic Cloud

Chiara Mastropietro, Andreas Burkert, Ben Moore

We use high resolution N-body/SPH simulations to study the hydrodynamical interaction between the Large Magellanic Cloud (LMC) and the hot halo of the Milky Way. We investigate whe…

astro-ph2008★ 2 cited

Modeling a high velocity LMC. The formation of the Magellanic Stream

Chiara Mastropietro

I use high resolution N-body/SPH simulations to model the new proper motion of the Large Magellanic Cloud (LMC) within the Milky Way (MW) halo and investigate the effects of gravit…

astro-ph2007★ 128 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…