000002500 001__ 2500
000002500 005__ 20160701171706.0
000002500 037__ $$aASTROimport-657
000002500 100__ $$aZorec, J.
000002500 245__ $$aEvolutionary status of Be stars
000002500 260__ $$c2004
000002500 520__ $$aFundamental parameters of nearly 50 field Be stars have been determined. Correcting these parameters from gravity darkening effects induced the fast rotation, we deduced the evolutionary phase of the studied stars. We show that the evolutionary phase at which appear the Be phenomenon is mass dependent: the smaller the stellar mass the elder the phase in the main sequence at which the Be phenomenon seem to appear. 
000002500 700__ $$a Frémat, Y.
000002500 700__ $$a Cidale, L.
000002500 773__ $$c327$$pSF2A-2004: Semaine de l'Astrophysique Francaise$$y2004
000002500 85642 $$ahttp://esoads.eso.org/abs/2004sf2a.conf..327Z
000002500 905__ $$apublished in
000002500 980__ $$aNONREF