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Newtonian Hydrodynamics of the Coalescence of Black Holes with Neutron Stars. I. Tidally Locked Binaries with a Stiff Equation of State
We present a detailed Newtonian study of the last stages of binary evolution of a black hole and a neutron star, when the components are separated by a few stellar radii. Our simulations are carried out using a three-dimensional smooth particle hydrodynamics (SPH) code. We calculate the gravitational radiation waveforms …