Title of article
The constant magnetic field of ξ1 CMa: geometry or slow rotation?
Author/Authors
Chloe Fourtune-Ravard، نويسنده , , Gregg A. Wade، نويسنده , , Wagner L. F. Marcolino، نويسنده , , Matthew Shultz، نويسنده , , Jason H. Grunhut، نويسنده , , Huib F. Henrichs، نويسنده , , the MiMeS Collaboration، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2010
Pages
2
From page
180
To page
181
Abstract
We report recent observations of the sharp-lined magnetic β Cep pulsator ξ1 CMa (= HD46328). The longitudinal magnetic field of this star is detected consistently, but it is not observed to vary significantly, during nearly 5 years of observation. In this poster we evaluate whether the constant longitudinal field is due to intrinsically slow rotation, or rather if the stellar or magnetic geometry is responsible.
Keywords
stars: early-type , stars: rotation , stars: individual (?1 CMa) , stars: magnetic fields
Journal title
Proceedings of the International Astronomical Union
Serial Year
2010
Journal title
Proceedings of the International Astronomical Union
Record number
667828
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