Free Access
Fig. 6
Upper panel: the [C ii] cooling rate per H atom as a function of the SFR for line-emitting gas associated with dense PDRs, cold H i gas, CO-dark H2 gas, and ionized gas. Lower panel: the [C ii] cooling rate as a function of Galactocentric radius for the different contributing ISM phases discussed in the text.
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.