3D Hydro-Simulation
Dust of a protoplanetary disc. The planet opens a gap and triggers a Rossby vortex.
3D Hydro-Simulation
Dust of a protoplanetary disc. The planet opens a gap and triggers a Rossby vortex.
Line-Integral-Convolution
Dust of a protoplanetary disc. The planet opens a gap and triggers a Rossby vortex.
3D Illustration of a Protoplanetary Disk
The vertical shear instability induces turbulence. Red: strength of the turbulence. Blue: large eddies in the disk plane. Pfeil & Klahr (2021)
Clumpy High-z Galaxy
Volume rendering of the higher density gas in a high-resolution simulation. The star-forming regions are illustrated in color in.
AGN evolution processes: black hole spin, accretion and feedback
Starting from an anti-aligned condition, the spin direction and magnitude of the central black hole in this simulation of an isolated Milky Way-like galaxy…
Clump Clusters in High-z Galaxies
(Line of sight gas surface density (linear scaling) of a simulated galaxy observed at an inclination of 60°)
The animation illustrates how clusters of many…
The animation illustrates how clusters of many…
Simulated "Odd Radio Circles" (SORCs)
A new kind of object has recently been discovered in radio observations, so-called "Odd Radio Circles" (ORCs).
Galaxy Cluster Simulations with a Spectral Cosmic Ray model
Formation of a massive galaxy cluster with acceleration of Cosmic Rays at shocks. We evolve a distribution function of CRs on-the-fly in the simulation which…
Effect of viscosity in the ICM
In the movies you can see the evolution of the main halo of a galaxy cluster for two different cases: the first one without the addition of physical viscosity…
