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Fig. 5

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Characteristics of the surviving fragment in model 1: a) orbital distance, b) mass of the fragment (solid line) and mass confined within the Hill radius (dashed line), c) radius of the fragment (solid line) and the Hill radius (dashed line), and d) integrated gravitational torque acting on the fragment in units of 8.6    ×    1040 g cm2 s-2.

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