Open Access

Fig. 9


Semimajor axis distribution and starting location of planets that have grown to gas giant masses (MP >100 M) in the ΣPr−2.1 and the planetesimal formation runs. We find that most massive planets end up at the inner edge of the disk. The total number of planets that have reached over 100 M in the ΣPr−2.1 runs is given as 41 out of 1961. This is heavily biased by the placement of the planetary seeds, however, which also occurs in far out regions with low planetesimal surface densities.

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