Fig. E.5.
Download original image
Comparison between our results and those from the FS. The differences are expressed as this study minus FS. Our silicon abundances are based on Si III. The microturbulence was adjusted by Hunter et al. (2009) to derive the same Si abundance for each star in the cluster (see Hunter et al. 2007; Trundle et al. 2007). Only the Δξ data for the stars with abundances from both this study and the FS are shown.
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.