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The ultimate fate of that debris, and the properties of the bright flare that is produced and observed, depends on a number of parameters, including the energy of the center of mass of the original star. Here we present the results of a set of smoothed particle hydrodynamics simulations in which a $1~M_\\odot $, $\\gamma = 5/3$ polytrope is disrupted by a $10^6 ~M_\\odot$ supermassive black hole. 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