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Fig. 4


Two-dimensional density structure of an isothermal disk (model 1) around the central binary star. The graph shows a local view around the binary. The computational grid extends from r = 0.25 AU to r = 2.0 AU. The white inner region lies inside the computational domain and is not covered by the grid. The positions of the primary and secondary are indicated by the gray dots. The Roche lobe of the secondary is also shown. (Online movie)

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