The magnetic field of AR UMa

Physics

Scientific paper

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Scientific paper

Optical spectropolarimetric observations of AR UMa in a low state of
activity show a very structured circular polarisation spectrum. The
strongest features in the phase-averaged spectrum can be modelled with a
dipole of strength Bd ~200-235 MG displaced from the centre
of the star by ~5-15% of the stellar radius along the magnetic axis.

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