000002896 001__ 2896
000002896 005__ 20160701171712.0
000002896 0247_ $$2DOI$$a10.1017/S1743921309030804
000002896 037__ $$aASTROimport-1053
000002896 100__ $$aHubrig, S.
000002896 245__ $$aNew magnetic field measurements of ß Cephei stars and slowly pulsating B stars
000002896 260__ $$c2009
000002896 520__ $$aWe present the results of the continuation of our magnetic survey with FORS 1 at the VLT of a sample of B-type stars consisting of confirmed or candidate ß Cephei stars and Slowly Pulsating B stars. Roughly one third of the studied ß Cephei stars have detected magnetic fields. The fraction of magnetic Slowly Pulsating B and candidate Slowly Pulsating B stars is found to be higher, up to 50%. We find that the domains of magnetic and non-magnetic pulsating stars in the H-R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence. 
000002896 700__ $$a Briquet, M.
000002896 700__ $$a De Cat, P.
000002896 700__ $$a Schöller, M.
000002896 700__ $$a Morel, T.
000002896 700__ $$a Ilyin, I.
000002896 773__ $$c389-390$$pCosmic Magnetic Fields: From Planets, to Stars and Galaxies$$v259$$y2009
000002896 85642 $$ahttp://esoads.eso.org/abs/2009IAUS..259..389H
000002896 905__ $$apublished in
000002896 980__ $$aNONREF