2619 20160701171708.0 ASTROimport-776 Zorec, J. 2007 Differential Rotation in Early-Type Stars Using 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. Frémat, Y. Domiciano de Souza, A. Active OB-Stars: Laboratories for Stellare and Circumstellar Physics 361 2007 542 http://esoads.eso.org/abs/2007ASPC..361..542Z published in NONREF