Free Access

Fig. 6.

image

Left panel: rotation profile Ω(r, θ) of 16 Cyg B corresponding to the MAP estimates of Ω0 and Ω1. The dashed line marks the bottom of the convective envelope. Right panel: distribution of the surface rotation rate as a function of the stellar co-latitude. The red shade represent probability densities. They have been normalised with respect to the rotational rate at fixed latitude. The black line marks the mode of the corresponding density, obtained from a Gaussian mixture model. The long-dash line shows the associated 68.3% credible interval. The short-dash line shows the model corresponding to the MAP estimates of Ω0 and Ω1.

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.