Fig. 3.
Download original image
Left panel: Fractions of CL, BS, RIN, and ITL passive galaxies as a function of stellar mass. Top panel: All morphological types; central and bottom panels: Early and late types, respectively, for CL and BS galaxies. Right panel: Fraction of recently strongly quenched galaxies. Types of galaxies are presented as shown in the left panel.
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.