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Published online by Cambridge University Press: 20 January 2011
The ANTARES code (A Numerical Tool for Astrophysical RESearch) is designed for doing 1D,2D and 3D stellar (radiation-, magneto-) hydrodynamics with realistic microphysics,applying various high-resolution numerical schemes, optionally local grid refinement andworks with rectilinear or spherical coordinates.– We present results on turbulent solargranulation flows which have been done in 2D and 3D and comment on our simulations of thepulsation-convection interaction in Cepheid variables, presently 2D.