000002659 001__ 2659
000002659 005__ 20160701171708.0
000002659 037__ $$aASTROimport-816
000002659 100__ $$aZorec, J.
000002659 245__ $$aOn the frequency of field galactic Be stars
000002659 260__ $$c2005
000002659 520__ $$aSince Be stars belong to the high velocity tail of a single B star velocity distribution, the appearance of the Be phenomenon must be independent of the stellar mass. In the present paper we show that the shape of the distribution of the number fraction N(Be)/N(Be+B) against the spectral type can be explained in terms of the Balmer line emission efficiency as a function of the effective temperature. 
000002659 700__ $$a Frémat, Y.
000002659 773__ $$c361$$pSF2A-2005: Semaine de l'Astrophysique Francaise$$y2005
000002659 85642 $$ahttp://esoads.eso.org/abs/2005sf2a.conf..361Z
000002659 905__ $$apublished in
000002659 980__ $$aNONREF