Relation between the galaxy stellar mass and its CO luminosity. The color code is the same as in Fig. 1. In both panels the straight line corresponds to the fit of the relation for the field galaxies with LIR < 2 × 1011 L⊙ to allow comparison with the clusters. We show the uncertainties of the mass estimates for our new sample of cluster 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.