This article has an erratum: [https://doi.org/10.1051/0004-6361/201322052e]
Narrow ring perturbed by an outer planet. a) Normalized surface density profile viewed head-on, for the nominal case with μ = 0.002, ap = 75 AU and τO = 2 × 10-3 (run C). The planet’s location is marked by the ⊕ symbol; b) azimuthally averaged radial distribution of the geometrical cross-section as a function of particle sizes (as parameterized by their β ratio) for run C; c) same as b), but for a denser and more collisionally active disc with τ = 2 × 10-2 (run E); d) same as b), but for a more tenuous disc with τ = 5 × 10-5 (run D).
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.