The Kelvin-Helmholtz instability is simulated using Gadget (left) and Arepo (right). The resolution in both cases is 240x240, with Gadget using N_ngb = 16
Credit:
Paul Torrey, Harvard University
Center for Astrophysics
Institute for Theory and Computation
Reference:
“Moving Mesh Cosmology: Properties of Gas Disks“
Paul Torrey, Mark Vogelsberger, Debora Sijacki, Volker Springel,
Lars Hernquist (2011)