Fig. C.2.

Model of an unperturbed spiral galaxy. Upper panel: SFR as a function of the molecular gas surface density. Middle panel: SFR as a function of the stellar surface density. Lower panel: star formation efficiency with respect to the molecular gas as a function of the stellar surface density. The solid lines mark the observed relations found by Leroy et al. (2008).
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.