Fig. 13
Hα flux versus veiling for the Cha I members observed with GIRAFFE and UVES. The accretor candidates (10%WHα> 270 km s-1) are denoted by filled symbols, as in Fig. 11. All the stars with a significant veiling (r ≥ 0.5) turn out to be confirmed or possible accretors. The full line is a linear best fit to the data with r ≥ 0.25.
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.