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Published online by Cambridge University Press: 26 May 2016
I review recent progress in numerically simulating the formation and evolution of galaxies in hierarchically clustering universes. Special emphasis is given to results based on high-resolution gas dynamical simulations using the N-body hardware integrator GRAPE. Applications address the origin of the spin of disk galaxies, the structure and kinematics of damped Ly-α systems, and the origin of galaxy morphology and of galaxy scaling laws.