MAP and IAB acknowledge funding from the European Research Council for the FP7 ERC advanced grant project ECOGAL. This work used the DiRAC Complexity system, operated by the University of Leicester IT Services, which forms part of the STFC DiRAC HPC Facility (www.dirac.ac.uk). This equipment is funded by BIS National E-Infrastructure capital grant ST/K000373/1 and STFC DiRAC Operations grant ST/K0003259/1. DiRAC is part of the National E-Infrastructure. GL acknowledges financial support from PNP, PNPS, PCMI of CNRS/INSU, CEA and CNES, France. An implementation of the code can be downloaded from https://github.com/mapetkova/kernel-integration.Voronoi grids have been successfully used to represent density structures of gas in astronomical hyd...
The ionizing feedback of young massive stars is well known to influence the dynamics of the birth en...
Density discontinuities cannot be precisely modelled in standard formulations of smoothed particles ...
Ionising radiation is present in a variety of astrophysical problems, and it is particularly importa...
International audienceVoronoi grids have been successfully used to represent density structures of g...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
A Lagrangian scheme that combines Voronoi diagrams with smoothed particle hydrodynamics (SPH) for in...
We present the results of a study comparing density maps reconstructed by the Delaunay Tessellation ...
We present the results of a study comparing density maps reconstructed by the Delaunay Tessellation ...
We present the results of a study comparing density maps reconstructed by the Delaunay Tessellation...
Context. Probing the structure of complex astrophysical objects requires effective three-dimensional...
The DSMC method simulates a gas by three uncoupled steps: moving representative particles through a ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
AbstractSmoothed particle hydrodynamics (SPH) simulations are often initialized on a regular Cartesi...
International audienceWe present a study of density estimation, the conversion of discrete particle ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
The ionizing feedback of young massive stars is well known to influence the dynamics of the birth en...
Density discontinuities cannot be precisely modelled in standard formulations of smoothed particles ...
Ionising radiation is present in a variety of astrophysical problems, and it is particularly importa...
International audienceVoronoi grids have been successfully used to represent density structures of g...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
A Lagrangian scheme that combines Voronoi diagrams with smoothed particle hydrodynamics (SPH) for in...
We present the results of a study comparing density maps reconstructed by the Delaunay Tessellation ...
We present the results of a study comparing density maps reconstructed by the Delaunay Tessellation ...
We present the results of a study comparing density maps reconstructed by the Delaunay Tessellation...
Context. Probing the structure of complex astrophysical objects requires effective three-dimensional...
The DSMC method simulates a gas by three uncoupled steps: moving representative particles through a ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
AbstractSmoothed particle hydrodynamics (SPH) simulations are often initialized on a regular Cartesi...
International audienceWe present a study of density estimation, the conversion of discrete particle ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
The ionizing feedback of young massive stars is well known to influence the dynamics of the birth en...
Density discontinuities cannot be precisely modelled in standard formulations of smoothed particles ...
Ionising radiation is present in a variety of astrophysical problems, and it is particularly importa...