Fig. 11
Upper panel: ṀZ as a function of core mass for the enriched and non-enriched cases of the high-opacities simulations (Fig. 10, bottom). The planetesimal accretion rate of the enriched case increases when the core reaches the threshold value of 11 M⊕. Lower panel: ratio of capture radius to core radius as a function of core mass (same simulation as in the upper panel).
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