Fig. 4

LSD Stokes I (first panel), Q (second panel), U (third panel) and V (fourth panel) profiles of HD 24712. Rotational phases calculated according to our improved ephemeris (see Sect. 7) are indicated in the first panel. Relative to Stokes I, the vertical scale for the Stokes Q and U profiles has been expanded by a factor of 36. The scale for the Stokes V profiles has been expanded by a factor of 6. The error bars are on the order of the thickness of the lines, therefore they are not shown on the plots. The red lines represent the LSD profiles of REEs while the black lines show the LSD profiles of Fe-peak elements. All profiles were corrected for the mean radial velocity of the star.
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.