Fig. C.3.
Same as Fig. C.1, but for the subsample with peculiar nuclear regions. Due to the strong dust extinction, violent star formation, and significant contribution from an AGN, no kinematic radius is measured for NGC 1365. We note that no kinematic radius is provided for NGC 6902, as there are no clear kinematic signatures of a nuclear disc in this galaxy.
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.