000002660 001__ 2660
000002660 005__ 20160701171708.0
000002660 037__ $$aASTROimport-817
000002660 100__ $$aZorec, J.
000002660 245__ $$aEvolution of galactic field Be stars
000002660 260__ $$c2005
000002660 520__ $$aGalactic field Be stars were studied by taking into account the effects induced by fast rotation on their fundamental parameters. Fractional ages t/tMS (tMS = time spent in the MS) against stellar mass reveal that: a) Be stars spread over the whole interval 0
000002660 700__ $$a Frémat, Y.
000002660 700__ $$a Cidale, L.
000002660 773__ $$c359$$pSF2A-2005: Semaine de l'Astrophysique Francaise$$y2005
000002660 85642 $$ahttp://esoads.eso.org/abs/2005sf2a.conf..359Z
000002660 905__ $$apublished in
000002660 980__ $$aNONREF