Fig. C.1
Download original image
Average SFRBirth as a function of look-back time for galaxies grouped by bar strength (rows) and disk thickness (columns). Each colored line represents the six radial bins in terms of hd. Galaxies with stronger bars tend to exhibit earlier and more centrally concentrated star formation, while those with thicker disks generally show higher SFRBirth for the same radial bin.
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.