Free Access

Fig. 17.

image

Comparison between the trend of overshoot with stellar mass for models in this paper and that reported by Claret & Torres (2017) and Claret & Torres (2018). The dotted lines show the range of overshoot found to be acceptable solutions for all systems in this study (and where members of each pair have the same overshooting parameter and MLT mixing length parameters. The square symbols show the best fits from Claret & Torres (2017) using the A09 mixture.

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.