SIMBAD references

2008MNRAS.388.1079I - Mon. Not. R. Astron. Soc., 388, 1079-1088 (2008/August-2)

Hydrodynamical adaptive mesh refinement simulations of turbulent flows - I. Substructure in a wind.

IAPICHINO L., ADAMEK J., SCHMIDT W. and NIEMEYER J.C.

Abstract (from CDS):

The problem of the resolution of turbulent flows in adaptive mesh refinement (AMR) simulations is investigated by means of three-dimensional (3D) hydrodynamical simulations in an idealized setup, representing a moving subcluster during a merger event. AMR simulations performed with the usual refinement criteria based on local gradients of selected variables do not properly resolve the production of turbulence downstream of the cluster. Therefore, we apply novel AMR criteria which are optimised to follow the evolution of a turbulent flow. We demonstrate that these criteria provide a better resolution of the flow past the subcluster, allowing us to follow the onset of the shear instability, the evolution of the turbulent wake and the subsequent back-reaction on the subcluster core morphology. We discuss some implications for the modelling of cluster cold fronts.

Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): hydrodynamics - instabilities - turbulence - methods: numerical - galaxies: clusters: general

Simbad objects: 2

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