000002658 001__ 2658
000002658 005__ 20160701171708.0
000002658 037__ $$aASTROimport-815
000002658 100__ $$aZorec, J.
000002658 245__ $$aAchernar can be a differential rotator
000002658 260__ $$c2005
000002658 520__ $$aWe take advantage of interferometric measurements of Achernar to inquire on its internal rotational law. The reinterpretation of interferometric data and the use of fundamental parameters corrected for gravitational darkening effects and 2D-models of internal stellar structures, lead us to the conclusion that the star could not be a rigid, near critical, rotator but a differential rotator with the core rotating ˜3 times faster than the surface. 
000002658 700__ $$a Domiciano de Souza, A.
000002658 700__ $$a Frémat, Y.
000002658 700__ $$a Vakili, F.
000002658 773__ $$c363$$pSF2A-2005: Semaine de l'Astrophysique Francaise$$y2005
000002658 85642 $$ahttp://esoads.eso.org/abs/2005sf2a.conf..363Z
000002658 905__ $$apublished in
000002658 980__ $$aNONREF