Magnetic field structure of slow CP-rotators: HD 9996 and HD 188041

Details Magnetic field structure of slow CP-rotators: HD 9996 and HD 188041 Magnetic field structure of slow CP-rotators: HD 9996 and HD 188041

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap.....51..242g&link_type=abstract

Astrophysics, Volume 51, Issue 2, pp.242-249

Astronomy and Astrophysics

Astrophysics

2

Stars, Magnetic Fields &Mdash, Individual, Hd 9996, Hd 188041

Scientific paper

This is the final paper on a study of the magnetic field structure of CP stars with long rotation periods. It is first demonstrated that the orientation and strength of the magnetic field have no effect on their rotation velocity. The orientation of the dipole structures in slow magnetic rotators is shown to be random, as it is in fast rotators. The hypothesis that magnetic stars are slowed down under the influence of the magnetic field is called into question. The origin of CP stars is probably related to their initial slow rotation.

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