Fig. 19
Hα line of Mon-000824 as a function of rotational phase, indicated in each plot. This star was not observed by CoRoT in 2011, and we used the photometric period (7.05 days) obtained in 2008, when the star presented an AA Tau-like light curve, to calculate the rotational phases. This star is a candidate to be in the unstable accretion regime in 2011.
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.