Free Access

Fig. 10


The width of the cross-correlation function as a function of each star’s V − Ks colour index. The top panel shows the full sample, including rapid rotators and the lower panel shows the zoomed region to highlight the slow rotators. The red solid curves represent our best fit to the lower boundary for the slowest rotators, along with the 1σ uncertainties shown by the dashed curves.

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.