Zorec, J. ; Frémat, Y. ; Cidale, L.

published in SF2A-2005: Semaine de l'Astrophysique Francaise, pp. 359 (2005)

Abstract: Galactic 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

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