Fig. 15

Factor
as a function of the core mass for different planetesimal sizes. The plot
corresponds to the case of a disk ten times more masive than the MMSN and
km when planetesimal
coagulation and fragmentation are considered. The black dashed line corresponds to
the evolution of the term (RP/RH)1
/ 2, where RP is the radius of the
planet. (Color version online.)
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