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1. Superrechner in der Kosmologie

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2. Physical viscosity in smoothed particle hydrodynamics simulations of galaxy clusters

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3. E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh. ArXiv e-prints, 0901.4107, MNRAS

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4. Cosmological SPH simulations: A hybrid multi-phase model for star formation

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5. The impact of early dark energy on non-linear structure formation

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6. E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh. ArXiv e-prints, 0901.4107, MNRAS

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7. An analytical model for the history of cosmic star formation

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8. Preprint typeset using LATEX style emulateapj v. 9/08/03 THE SPEED OF THE ‘BULLET ’ IN THE MERGING GALAXY CLUSTER 1E0657–56

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9. Title not available

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10. cosmological simulation code GADGET

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