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Fig. 17
Evolution of the mass (top panel) and its fraction with respect to the final mass (bottom panel) of the resulting planets thatsurvived inside the IHZ at 100 Myr (solid lines) and 1 Gyr (dotted lines) in S1 with tide and GR (orange curves), in S2 without tide and GR (cyan curves), and in S2 with tide and GR (red curves).
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