Fig. 6
X-ray luminosity function of Class III stars (comprised 3 DDs). For comparison we added the curves of Class III stars in L1688 from DROXO, both corrected (solid gray line) and total sample (dotted gray line, see Pillitteri et al. 2010), and L1641 (solid light blue line, Pillitteri et al. 2013). Class III stars around ρ Ophiuchi shows less luminosities and a larger range of values.
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.