Fig. 5
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Initial planetesimals surface density profiles for 10 discs, which were selected using the quantiles of the disc mass distribution,to be representative of the entire population. The top and bottom grey lines thus show the most and least massive disc. The red line is the minimum-mass solar nebula (MMSN, Weidenschilling 1977; Hayashi 1981), while the blue line is the minimum-mass extrasolar nebula (Chiang & Laughlin 2013, CL13).
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