Fig. 1
⟨ Bz ⟩ and Hipparcos photometry variations of HD 133652. Top: ⟨ Bz ⟩ LSD measurements (red triangles) and the Balmer line measurements from Bohlender et al. (1993, filled circles with error bars). The solid blue line is the best-fit magnetic field variations (see Sect. 4.1). Bottom: the Hipparcos photometry variations with rotational phase. The dotted blue line is the best-fit sinusoid to the observations.
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