000002562 001__ 2562
000002562 005__ 20160701171707.0
000002562 037__ $$aASTROimport-719
000002562 100__ $$aFrémat, Y.
000002562 245__ $$aCNO abundance determination in massive fast rotating stars
000002562 260__ $$c2008
000002562 520__ $$aBe stars are early-type Main Sequence objects which have shown at least once some emission in the hydrogen line series. Their most important characteristic is fast rotation, which on average reach ˜ 90% of the critical rate, i.e. O/O_{c} %˜ 0.90. Since a number of them have masses M > 15 M_?, they are ideal targets to study the effects of rotational mixing on the atmospheric CNO abundance and to perform comparisons with the predictions obtained from recent evolutionary models with rotation. 
000002562 700__ $$a Zorec, J.
000002562 700__ $$a Martayan, C.
000002562 700__ $$a Lanz, T.
000002562 773__ $$c53-53$$pRevista Mexicana de Astronomia y Astrofisica Conference Series$$v33$$y2008
000002562 85642 $$ahttp://esoads.eso.org/abs/2008RMxAC..33...53F
000002562 905__ $$apublished in
000002562 980__ $$aNONREF