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Fig. 2


Top: comparison of the Stokes V profiles obtained by selecting photospheric lines of low (red thin line) and high (green thin line) magnetic sensitivity for β UMa. The thick red and green lines represent a moving average over three spectral bins of the thin lines. Center: same figure for θ Leo. Bottom: same for α2 CVn. All profiles are normalized to the continuum level.

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

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