Free Access

Fig. 20

image

Model fits to the [Ca II] λ 7291 profiles corresponding to the FEROS spectra (2014 and December 2015 data, top and bottom panels, respectively). The computed profiles (in red line) were obtained combining different emission structures with different projected Keplerian rotational velocities (see Table 1). The [Ca II] λ 7291 line from November 2015 FEROS data could not be modelled since it is very noisy.

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.