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Fig. 4.
Gas density on the orbital plane for for models with the same orbital separation and mass ratio (a = 5 AU, q = 1), but different initial wind velocities (1 km s−1 and 12 km s−1). For clarity, the density scale here is different from the previous figures. For model Q1a5 (right) this figure is a close-up version of Fig. 3a.
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