Free Access

Fig. 11

thumbnail

Flux-flux relations for which MA11 identified two distinct populations in a sample of field stars (shown as solid lines). Our sample of Class III stars is shown with the same plotting symbols as in Fig. 4 and is located on the upper relation. It extends this “active branch” to lower fluxes. Linear regressions and standard deviation for the Class III detections are shown as dash-dotted and dotted lines as in Fig. 10.

This figure is made of several images, please see below:

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.