Fig. 14
Comparison of our results for the G-type eclipsing pair with theoretical PARSEC Z = 0.0103 isochrones on mass vs. absolute Kepler magnitude (top) and radius (bottom) planes. A good agreement is found for ages of 35 Myr (red line) and 3.16 Gyr (grey line). Stellar parameters predicted for the F1-type pulsator favour the former age.
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.