Evolution of the orbital distance of pebbles as they drift through a disc with an embedded 25 ME planet, where the radial velocity is fixed to − 1 × 10−5cs,0 (top) and − 3 × 10−5cs,0 (bottom). As the drift speed of the particles depends on the gas velocities, particles of different sizes cannot be blocked or drift through compared to the nominal case shown in Fig. 8. In particular, a slower gas flow allows for a more efficient particle trapping in the pressure bump generated by the planet.
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.