Fig. 1
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Differential mass distribution of the planetesimals formed near the initial disc substructure for the set of simulations with α = 5 × 10−4 drawn from the adopted initial mass function by Gerbig & Li (2023). There are 10 bins per decade in mass m and ΔN is the number of planetesimals in each bin. Each colour corresponds to one of the five simulations.
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