Fig. 1
Sketch illustrating pebble accretion in two different frames. a) Local frame: the co-moving frame is centred on the planet where the x-axis is pointing radially away from the star and the y-axis follows the orbital direction of the planet. Grey arrows purely indicate the gas velocity of the shearing flow, and the blue arrow shows the trajectory of the pebble, with the x-axis impact distance b and the y-axis velocity vy(b). b) Global frame: the planet orbits around the central star with a semi-major axis ap. The black arrow depicts the planet motion and the blue arrows illustrate the trajectories of pebbles that cross the orbit of 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.