Exploring the formation of multiple dust-trapping rings in the inner Solar System

Open Access

Fig. 3

Perturbed surface density of the HD_Bae simulation at the same snapshots represented in Fig. 2. The dashed lines indicate the radial position of the pressure bumps, i.e. the values of r for which η = 0 in Fig. 2. The dot-dashed line indicates the boundary of the damping region.

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.