000002621 001__ 2621
000002621 005__ 20160701171708.0
000002621 037__ $$aASTROimport-778
000002621 100__ $$aLevenhagen, R. S.
000002621 245__ $$aMetallicity vs. Be Phenomenon Relation in the Solar Neighborhood
000002621 260__ $$c2007
000002621 520__ $$aFast rotation seems to be the mayor factor to trigger the Be phenomenon. Surface fast rotation can be favored by initial formation conditions, such as abundance of metals. We have observed 118 Be stars up to the apparent magnitudes V=9 mag. Models of fast rotating atmospheres and evolutionary tracks were used to interpret the stellar spectra and to determine the stellar fundamental parameters. Since the studied stars are formed in regions that are separated enough to imply some non negligible gradient of galactic metallicity, we study the effects of possible incidence of this gradient on the nature as rotators of the studied stars. 
000002621 700__ $$a Leister, N. V.
000002621 700__ $$a Zorec, J.
000002621 700__ $$a Frémat, Y.
000002621 773__ $$c457$$pActive OB-Stars: Laboratories for Stellare and Circumstellar Physics$$v361$$y2007
000002621 85642 $$ahttp://esoads.eso.org/abs/2007ASPC..361..457L
000002621 905__ $$apublished in
000002621 980__ $$aNONREF