The constant magnetic field of xi 1 CMa: geometry or slow rotation?

Details The constant magnetic field of xi 1 CMa: geometry or slow rotation? The constant magnetic field of xi 1 CMa: geometry or slow rotation?

2010-09-18

arxiv.org/abs/1009.3565v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Scientific paper

We report recent observations of the sharp-lined magnetic beta Cep pulsator xi 1 CMa (= HD 46328). The longitudinal magnetic field of this star is detected consistently, but it is not observed to vary strongly, during nearly 5 years of observation. In this poster we evaluate whether the nearly constant longitudinal field is due to intrinsically slow rotation, or rather if the stellar or magnetic geometry is responsible.

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