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Fig. 14


Growth tracks of planets starting at several different initial positions in a disc that is already 1.5 Myr old for pebble-isolation masses given by Lambrechts et al. (2014) in Eq. (1) and for the new-found pebble isolation mass Miso in Eq. (26). The initial growth phase is the same for both isolation masses, so the growth tracks diverge only when the pebble-isolation mass (Eq. (1)) is reached, marked by the dots. The solid lines indicate pebble accretion, while the dashed lines mark gas accretion.

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