000002620 001__ 2620
000002620 005__ 20160701171708.0
000002620 037__ $$aASTROimport-777
000002620 100__ $$aZorec, J.
000002620 245__ $$aRotation in the ZAMS: Be and Bn stars
000002620 260__ $$c2007
000002620 520__ $$aWe show that Be stars belong to a high velocity tail of a single B-type star rotational velocity distribution in the MS. This implies that: 1) the number fraction N(Be)/N(Be+B) is independent of the mass; 2) Bn stars having ZAMS rotational velocities higher than a given limit might become Be stars. 
000002620 700__ $$a Frémat, Y.
000002620 700__ $$a Martayan, C.
000002620 700__ $$a Cidale, L. S.
000002620 700__ $$a Torres, A. F.
000002620 773__ $$c539$$pActive OB-Stars: Laboratories for Stellare and Circumstellar Physics$$v361$$y2007
000002620 85642 $$ahttp://esoads.eso.org/abs/2007ASPC..361..539Z
000002620 905__ $$apublished in
000002620 980__ $$aNONREF