Abstract Smoothed Particle Hydrodynamics (SPH) is a relatively new meshless numerical
approach which has attracted significant attention in the last two decades. Compared with …

Direct images of protoplanets embedded in disks around infant stars provide the key to
understanding the formation of gas giant planets such as Jupiter. Using the Subaru …

We present two new Lagrangian methods for hydrodynamics, in a systematic comparison
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …

This paper describes the open-source code Enzo, which uses block-structured adaptive
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …

The design and implementation of a new framework for adaptive mesh refinement
calculations are described. It is intended primarily for applications in astrophysical fluid …

The methods in the Gasoline2 smoothed particle hydrodynamics (SPH) code are described
and tested. Gasoline2 is the most recent version of the Gasoline code for parallel …

We present an implementation of smoothed particle hydrodynamics (SPH) with improved
accuracy for simulations of galaxies and the large-scale structure. In particular, we …

We present Phantom, a fast, parallel, modular, and low-memory smoothed particle
hydrodynamics and magnetohydrodynamics code developed over the last decade for …

Many white dwarf stars show signs of having accreted smaller bodies, implying that they
may host planetary systems. A small number of these systems contain gaseous debris discs …

Protoplanetary disks (PPDs) are believed to accrete onto their central T Tauri star because
of magnetic stresses. Recently published shearing box simulations indicate that Ohmic …