Free Access
Fig. 5
Dynamical evolution of a simulation similar to the one shown in Fig. 4, but using Speb = 2.5. The larger pebble flux leads to faster growth and thus larger planets via pebble accretion. Even before the disk dissipates, planetary embryos collide and form massive bodies.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.