Upper panels: as in Fig. 4, but here, the color code indicates different wind parameters λ of the galaxies that reproduce the MZ relations. Lower panels: distribution of the predicted passive galaxies (red histogram) and star-forming galaxies (blue histogram) that reproduced the MZ relation in terms of the wind parameter λ of galaxies. In the left panel we adopt a Chabrier (2003) IMF, whereas in the right panel a Salpeter (1955) IMF is adopted.
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.