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19972008
most citedNumerical simulations of compressively driven interstellar turbulence: I. Isothermal gas

229 citations · 709 across the 11 of their papers we have counts for

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astro-ph2008229 cited

Numerical simulations of compressively driven interstellar turbulence: I. Isothermal gas

Wolfram Schmidt, Christoph Federrath, Markus Hupp +2

We performed numerical simulations of supersonic isothermal turbulence driven by mostly compressive large-scale forcing, using both a static grid and adaptive mesh refinement with…

astro-ph200897 cited

Hydrodynamical adaptive mesh refinement simulations of turbulent flows - II. Cosmological simulations of galaxy clusters

L. Iapichino, J. C. Niemeyer

The development of turbulent gas flows in the intra-cluster medium and in the core of a galaxy cluster is studied by means of adaptive mesh refinement (AMR) cosmological simulation…

astro-ph200844 cited

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

L. Iapichino, J. Adamek, W. Schmidt +1

The problem of the resolution of turbulent flows in adaptive mesh refinement (AMR) simulations is investigated by means of 3D hydrodynamical simulations in an idealised setup, repr…

astro-ph2007177 cited

A three-dimensional deflagration model for Type Ia supernovae confronted with observations

F. K. Roepke, W. Hillebrandt, W. Schmidt +3

A simulation of the thermonuclear explosion of a Chandrasekhar-mass C+O white dwarf, the most popular scenario of a type Ia supernova (SN Ia), is presented. The underlying modeling…

astro-ph200620 cited

C+O detonations in thermonuclear supernovae: Interaction with previously burned material

A. Maier, J. C. Niemeyer

In the context of explosion models for Type Ia Supernovae, we present one- and two-dimensional simulations of fully resolved detonation fronts in degenerate C+O White Dwarf matter…

astro-ph2006118 cited

A localised subgrid scale model for fluid dynamical simulations in astrophysics II: Application to type Ia supernovae

W. Schmidt, J. C. Niemeyer, W. Hillebrandt +1

The dynamics of the explosive burning process is highly sensitive to the flame speed model in numerical simulations of type Ia supernovae. Based upon the hypothesis that the effect…