Open Access
Fig. 7
Mass distribution of red giant branch stars where the rotational multiplet components have been identified. The darkness of the dots is positively correlated with the number of superimposed dots. Left panel: mass as a function of the radius. Right panel: mass as a function of the mixed-mode density.
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.