Open Access

Fig. 8

image

Cumulative function of planetary masses within 1 au for the four different synthetic populations from Fig. 5. The y-axis shows how many planets for each density profile are above the current planetary mass, normalized by the total number for planets in each population. The planets that have formed in the ΣPr−0.9 run are shown in green, the ΣPr−1.5 population is shown in orange, and the ΣPr−2.1 population is shown in blue. The dynamic planetesimal formation population is shown in black.

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