Free Access

Fig. 10.


O abundances as functions of effective temperature (upper panel) and against Al abundances for three of our clusters (bottom panels) determined by the BACCHUS code with the APOGEE DR14 uncalibrated Teff and log g (black dots) and by the ASPCAP pipeline (uncalibrated values, red triangles). The oxygen trend is slightly positive in contrast to Fig. 7. Moreover, almost no O dispersion nor anticorrelation is observed, which cast some doubts on the stellar parameters.

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.