Fig. 10.
Download original image
Normalized Ca II H&K emission (
) as a function of Prot. ‘D’ and ‘P’ rotators are omitted from the plot. The relation from Astudillo-Defru et al. (2017a) is overplotted in grey. To illustrate the offset with that relation for our fully convective stars in the unsaturated regime, we also show the best-fit power law for 18 ‘S’ rotators with M⋆ ≤ 0.35 M⊙ and Prot > 40 d in dashed red lines.
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.