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Fig. 5.
Density of the gas for models Q2a4v1 and Q2a4v1Ω after 9.5 orbital periods. The images on the left show the density and velocity field in the inertial frame in the orbital plane (z = 0). The images on the right show the same quantities, but on the y = 0 plane. The dashed lines correspond to the Roche-lobes of the stars.
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