Linking planetary embryo formation to planetesimal formation - I. The effect of the planetesimal surface density in the terrestrial planet zone

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Fig. 9

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Active number of planetary embryos and mass in planetary embryos over time for the LIPAD runs from Figs. 2–4. We also show the fraction (M_Emb∕M_D) of mass in embryos over the final planetesimal mass that entered the disk after 1 Myr.

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