The interplay between pebble and planetesimal accretion in population synthesis models and its role in giant planet formation

Open Access

Fig. 2

Formation tracks of a planet during 2 Gyr with pebble fractions f_peb from 0 to 1 in increments of 0.1 (colours) using the same disk that gives rise to the encircled planets in Fig. 1. The tracks of the four cases (f_peb = 0, 0.3, 0.7, 1) shown in Fig. 1 are again marked by a red circle.

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