Dust ring and gap formation by gas flow induced by low-mass planets embedded in protoplanetary disks - I. Steady-state model

Open Access

Fig. 16

Schematic illustrations of our model for the dust ring and gap formation. The planet-induced gas flow is in the flow-shear regime (panel a) and in the flow-headwind regime (panel b) to form dust substructures.

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.