000002771 001__ 2771
000002771 005__ 20160701171710.0
000002771 037__ $$aASTROimport-928
000002771 100__ $$aHubrig, S.
000002771 245__ $$aFirst Magnetic Field Models for Recently Discovered Magnetic ß Cephei and Slowly Pulsating B Stars
000002771 260__ $$c2012
000002771 520__ $$aDespite of the importance of magnetic fields for the full understanding of the properties of pulsating ß Cephei and slowly pulsating B (SPB) stars,  these fields have scarcely been studied over the rotation cycle until now. During the past two years we have obtained multi-epoch polarimetric spectra of several ß Cephei and SPB stars with FORS 2 at the Very Large Telescope and SOFIN at the Nordic Optical Telescope to search for a rotation period and to constrain the geometry of the magnetic field. The rotation periods and  magnetic field geometries were determined for three ß Cephei stars, E1 CMa, 15 CMa, and V1449 Aql, the candidate ß Cephei star a Pyx, and the SPB star 33 Eri. 
000002771 700__ $$a Schöller, M.
000002771 700__ $$a Ilyin, I.
000002771 700__ $$a Briquet, M.
000002771 700__ $$a Morel, T.
000002771 700__ $$a De Cat, P.
000002771 773__ $$c307$$pProgress in Solar/Stellar Physics with Helio- and Asteroseismology$$v462$$y2012
000002771 85642 $$ahttp://esoads.eso.org/abs/2012ASPC..462..307H
000002771 905__ $$apublished in
000002771 980__ $$aNONREF