000002271 001__ 2271
000002271 005__ 20160706142504.0
000002271 0247_ $$2DOI$$a10.1088/2041-8205/726/1/L5
000002271 037__ $$aASTROimport-428
000002271 100__ $$aHubrig, S.
000002271 245__ $$aFirst Magnetic Field Models for Recently Discovered Magnetic ß Cephei and Slowly Pulsating B Stars
000002271 260__ $$c2011
000002271 520__ $$aIn spite of recent detections of magnetic fields in a number of ß Cephei and slowly pulsating B (SPB) stars, their impact on stellar rotation, pulsations, and element diffusion has not yet been sufficiently studied. The reason for this is the lack of knowledge of rotation periods, the magnetic field strength distribution and temporal variability, and the field geometry. New longitudinal field measurements of four ß Cephei and candidate ß Cephei stars, and two SPB stars were acquired with FORS 2 at the Very Large Telescope. These measurements allowed us to carry out a search for rotation periods and to constrain the magnetic field geometry for four stars in our sample. Based on observations obtained at the European Southern Observatory (ESO programme 084.D-0230(A)).
000002271 700__ $$aIlyin, I.
000002271 700__ $$aSchöller, M.
000002271 700__ $$aBriquet, M.
000002271 700__ $$aMorel, T.
000002271 700__ $$aDe Cat, P.
000002271 773__ $$cL5$$i1$$pThe Astrophysical Journal$$v726$$y2011
000002271 85642 $$ahttp://esoads.eso.org/abs/2011ApJ...726L...5H
000002271 905__ $$apublished in
000002271 980__ $$aREFERD