Open Access
Fig. 13.
Download original image
Top: spatial distribution of the stars of the open cluster NGC 2516. Bottom: Gaia DR3 combined radial velocities as a function of G magnitude for the stars of the open cluster NGC 2516. The correction of the magnitude trend of the hot stars recommended in Blomme et al. (2023) is applied.
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.