Free Access
Fig. 18
Period–magnitude diagram for the known and the newly discovered eclipsing binaries of our sample, showing a prominent concentration of early type EBs in short-period orbits and a distinctive tail of luminous EBs towards longer periods. All four AFG-type EBs exhibit periods over ~30 days.
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.