Figure 5
The geometry adopted for HD 133880. The vertical axis is the rotation axis of the star. The angle between the line of sight and the rotation axis is i= 55°. The angle between the rotation axis and the magnetic field axis is β= 78°. The left-hand panel depicts an orientation where the positive magnetic pole is closest to the line of sight (φ= 0.537) and the right-hand panel is when the negative magnetic pole is nearer alignment with the line of sight (φ= 0.037). The bands used for dividing the abundance distribution are shown as solid lines and are normal to the magnetic field axis.

The geometry adopted for HD 133880. The vertical axis is the rotation axis of the star. The angle between the line of sight and the rotation axis is i= 55°. The angle between the rotation axis and the magnetic field axis is β= 78°. The left-hand panel depicts an orientation where the positive magnetic pole is closest to the line of sight (φ= 0.537) and the right-hand panel is when the negative magnetic pole is nearer alignment with the line of sight (φ= 0.037). The bands used for dividing the abundance distribution are shown as solid lines and are normal to the magnetic field axis.

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