000002619 001__ 2619
000002619 005__ 20160701171708.0
000002619 037__ $$aASTROimport-776
000002619 100__ $$aZorec, J.
000002619 245__ $$aDifferential Rotation in Early-Type Stars
000002619 260__ $$c2007
000002619 520__ $$aUsing 2D models of rotating stars, the interferometric measurements of aEri and its fundamental parameters corrected for gravitational darkening effects we infer that the star might have a core rotating 2.7 times faster than the surface. We explore the consequences on spectral lines produced by surface differential rotation combined with the effects due to a kind of internal differential rotation with rotational energies higher than allowed for rigid rotation which induce geometrical deformations that do not distinguish strongly from those carried by the rigid rotation. 
000002619 700__ $$a Frémat, Y.
000002619 700__ $$a Domiciano de Souza, A.
000002619 773__ $$c542$$pActive OB-Stars: Laboratories for Stellare and Circumstellar Physics$$v361$$y2007
000002619 85642 $$ahttp://esoads.eso.org/abs/2007ASPC..361..542Z
000002619 905__ $$apublished in
000002619 980__ $$aNONREF