Diversity in the outcome of dust radial drift in protoplanetary discs

Free Access

Fig. B.1

Open with DEXTER Download original image

Same as Fig. 1 but with migration for s>s_opt. Taking into account the migration only marginally affects the temperature profile and subsequent migration of the remaining grains. The 2 dotted lines show the envelope of the models without migration (displayed in Fig. 1) for comparison.

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.