Model magnetic fields of CP stars
with long rotation periods

Yu.V. Glagolevskij, Special Astrophysical Observatory of Russian AS, Nizhnij Arkhyz 369167, Russia.
e-mail: glagol@sao.ru
E. Gerth, D-14471 Potsdam, Gontardstr 130, Germany.
e-mail: ewald-gerth@t-online.de

Abstract
The formerly adopted hypothesis of loss of rotational momentum in presence of magnetic fields seems to be contradicted by some recently investigated magnetic CP stars.

Key words: stars: magnetic fields – rotation – long periods

Preprint of an article submitted to: Magnetic Stars, Proc. Internat. Conf. SAO, Nizhnij Arkhyz, Russia, 28 August - 1 September 2006.
Poster available by    www.ewald-gerth.de/118pos.pdf .