Turbulent Motions and Shocks Waves in Galaxy Clusters simulated with AMR (2009)
Vazza, F., Brunetti, G., Kritsuk, A., Wagner, R., Gheller, C., Norman, M .
We have implemented an Adaptive Mesh Refinement criterion explicitly designed to increase spatial resolution around discontinuities in the velocity field in ENZO cosmological simulations. With this...
Hydrodynamics and Stability of Galactic Cooling Flows (2007)
Kritsuk Bohringer, A. Kritsuk, H. Bohringer, E. Muller
Using numerical techniques we studied the global stability of cooling flows in giant elliptical galaxies. As an initial equilibrium state we choose the hydrostatic gas recycling model (Kritsuk 1996)....
Convective cores in galactic cooling flows (2000)
Kritsuk, A., Plewa, T., Mueller, E.
We use hydrodynamic simulations with adaptive grid refinement to study the dependence of hot gas flows in X-ray luminous giant elliptical galaxies on the efficiency of heat supply to the gas. We...
Hydrodynamics and stability of galactic cooling flows (1998)
Kritsuk, A., Boehringer, H., Mueller, E.
Using numerical techniques we studied the global stability of cooling flows in giant elliptical galaxies. As an initial equilibrium state we choose the hydrostatic gas recycling model (Kritsuk 1996)....