activity
20082014
most citedSimulations of the formation and evolution of isolated dwarf galaxies

83 citations · 338 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2014★ 35 cited

Numerical simulations of dwarf galaxy merger trees

Annelies Cloet-Osselaer, Sven De Rijcke, Bert Vandenbroucke +3

We investigate the evolution of dwarf galaxies using N -body/SPH simulations that incorporate their formation histories through merger trees constructed using the ex- tended Press-…

astro-ph.GA2014★ 43 cited

Gaseous infall triggering starbursts in simulated dwarf galaxies

Robbert Verbeke, Sven De Rijcke, Mina Koleva +3

Using computer simulations, we explored gaseous infall as a possible explanation for the starburst phase in Blue Compact Dwarf galaxies. We simulate a cloud impact by merging a sph…

astro-ph.GA2014★ 24 cited

On the origin of bursts in blue compact dwarf galaxies: clues from kinematics and stellar populations

M. Koleva, S. De Rijcke, W. W. Zeilinger +3

Blue compact dwarf galaxies (BCDs) form stars at, for their sizes, extraordinarily high rates. In this paper, we study what triggers this starburst and what is the fate of the gala…

astro-ph.CO2013★ 51 cited

Stellar orbits and the survival of metallicity gradients in simulated dwarf galaxies

Joeri Schroyen, Sven De Rijcke, Mina Koleva +2

We present a detailed analysis of the formation, evolution, and possible longevity of metallicity gradients in simulated dwarf galaxies. Specifically, we investigate the role of po…

astro-ph.CO2013★ 29 cited

New composition dependent cooling and heating curves for galaxy evolution simulations

Sven De Rijcke, Joeri Schroyen, Bert Vandenbroucke +4

In this paper, we present a new calculation of composition-dependent radiative cooling and heating curves of low-density gas, intended primarily for use in numerical simulations of…

astro-ph.CO2013★ 8 cited

Physics of a partially ionized gas relevant to galaxy formation simulations -- the ionization potential energy reservoir

Bert Vandenbroucke, Sven De Rijcke, Joeri Schroyen +1

Simulation codes for galaxy formation and evolution take on board as many physical processes as possible beyond the standard gravitational and hydrodynamical physics. Most of this…

astro-ph.CO2012★ 22 cited

The degeneracy between star-formation parameters in dwarf galaxy simulations and the Mstar-Mhalo relation

Annelies Cloet-Osselaer, Sven De Rijcke, Joeri Schroyen +1

We present results based on a set of N-Body/SPH simulations of isolated dwarf galaxies. The simulations take into account star formation, stellar feedback, radiative cooling and me…

astro-ph.GA2011★ 43 cited

Simulations of the formation and evolution of isolated dwarf galaxies - II. Angular momentum as a second parameter

Joeri Schroyen, Sven De Rijcke, Sander Valcke +2

We show results based on a large suite of N-Body/SPH simulations of isolated, flat dwarf galaxies, both rotating and non-rotating. The main goal is to investigate possible mechanis…

astro-ph2008★ 83 cited

Simulations of the formation and evolution of isolated dwarf galaxies

Sander Valcke, S. De Rijcke, H. Dejonghe

We present new fully self-consistent models of the formation and evolution of isolated dwarf galaxies. We have used the publicly available N-body/SPH code HYDRA, to which we have a…