Free Access

Fig. 3

image

Effect of numerical resolution on the planet migration (upper panel) and planet eccentricity (lower panel). The trapping position of the planet is not sensitive to the resolution while the trapping time can vary. In HR2, because the outer boundary is at 1.3 (Table 1), we set the planet slightly inward of the other two models to avoid numerical issues.

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.