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

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.

preprint2010arXivOpen access
C. Fourtune-RavardG. A. WadeW. MarcolinoM. ShultzJ. GrunhutH. F. Henrichsthe MiMeS Collaboration
astro-ph.SR
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Open access7 authors1 topic
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C. Fourtune-RavardG. A. WadeW. MarcolinoM. ShultzJ. GrunhutH. F. Henrichsthe MiMeS Collaboration

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