Simultaneous X-ray and optical variability of M dwarfs observed with eROSITA and TESS

Open Access

Fig. 2

Distribution of distances for the two subsamples that are X-ray brightest and the most X-ray variable defined in Sect. 3.4 as well as the entire M-dwarf sample in the TESS SCVZ described in Sect. 3.2.

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.