Online material
Appendix A: Additional material
Table A.1
Fundamental parameters of β Cephei and candidate
β Cephei stars with detected magnetic fields.
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Fig. A.1
An example of Stokes I and Stokes V spectra
observed at phase 0.648 in the wavelength region
λλ 4775–4800 containing several N ii spectral lines.
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| Open with DEXTER |
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Fig. A.2
Line profile variability of O ii λλ4699, 4705, 4710,
and He i λ4713 over the rotation cycle on SOFIN spectra.
The spectra are presented with phases increasing from bottom to top
and offset in the vertical direction for clarity.
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| Open with DEXTER |
© ESO, 2011
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