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Fig. 6


Numerical smoothed particle hydrodynamics simulation of an accretion disk in dynamical equilibrium for mass ratio 10-3 after 400 orbits. The solid curve represents the equatorial Roche lobes. The accretor has been marked by a small open circle. The dashed circles indicate the 3:1 (inner) and 2:1 (outer) resonances with the orbital period.

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