Free Access
Fig. 6.

Mass fraction formed in δt = 10 Myr in stars more massive than 8.0 M⊙ relative to the total initial mass in the IGIMF models (Eq. (14)) shown in dependence of the SFR and [Fe/H]. The canonical IMF is depicted as the horizontal black line (F80 ≈ 0.22).
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.