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Fig. 13

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Evolution of the angle between the angular momentum of the disk and that of: (i) gas at three different volume densities (dash-dotted: n0, dashed: 0.2 × n0, dotted: n = 0.04 × n0); (ii) newly born tail stars younger than 10 Myr (solid line); and (iii) all young tail stars with ages younger than 200 Myr (thick solid line).

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