Free Access

Fig. 19

image

Dependence of the velocity component V on for K–M dwarfs: solid points represent subgroups of MCC stars, defined by the orbital vertical height Zmax, and open squares are for synthetic stellar subsamples of the Besançon model, defined by age. The black thick line is a linear fit to the MCC points, with uncertainty limits shown as gray lines. The dotted blue line is a linear fit to the model data.

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.