We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic chemodynamics code GCD+. The applied scheme includes implementations of the artificial viscosity switch and artificial thermal conductivity proposed by Morris & Monaghan, Rosswog & Price and Price to model discontinuities and Kelvin-Helmholtz instabilities more accurately. We first present hydrodynamics test simulations and contrast the results to runs undertaken without artificial viscosity switch or thermal conduction. In addition, we also explore the different levels of smoothing by adopting larger or smaller smoothing lengths, i.e. a larger or smaller number of neighbour particles, Nnb. We demonstrate that the new version of GCD+ is capable ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our tree N-body/SPH galactic ch...
We present an implementation of smoothed particle hydrodynamics (SPH) with improved accuracy for sim...
Smoothed particle hydrodynamics (SPH) is a Lagrangian method for solving the fluid equations that is...
We adapt the smoothed-particle hydrodynamics (SPH) technique to allow a multiphase fluid in which SP...
This paper investigates the hydrodynamic performances of an smoothed particle hydrodynamics (SPH) co...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
We present a novel implementation of smoothed particle hydrodynamics that uses the spatial derivativ...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our treeN-body/SPH galactic che...
We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our tree N-body/SPH galactic ch...
We present an implementation of smoothed particle hydrodynamics (SPH) with improved accuracy for sim...
Smoothed particle hydrodynamics (SPH) is a Lagrangian method for solving the fluid equations that is...
We adapt the smoothed-particle hydrodynamics (SPH) technique to allow a multiphase fluid in which SP...
This paper investigates the hydrodynamic performances of an smoothed particle hydrodynamics (SPH) co...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
We present a novel implementation of smoothed particle hydrodynamics that uses the spatial derivativ...
Given the importance of shear flows for astrophysical gas dynamics, we study the evolution of the Ke...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...
Aims. Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, ...