Fig. 5

HR diagram of NGC 3766. The estimated age of the cluster of ~31 Myr included the cool giant CD−60 3621 reported by Levesque et al. (2005) (filled circle). The isochrone curves are given by Bressan et al. (1993). Possible members of the clusters are denoted in ⋆ (blue) symbols and possible non-members (pnm) in filled ▴ (red).
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.