Fig. 21.
Download original image
Star formation efficiency. Upper panel: Star formation efficiency with respect to the molecular gas as a function of the angular velocity Ω. The lines correspond to an outlier-resistant linear bisector fit and its dispersion. Lower panel: Star formation efficiency with respect to the molecular gas as a function of the turbulent velocity dispersion. The fit only applies to the SF galaxies.
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.