[en] In the framework of the Gaia-ESO survey we have determined the
fundamental parame-
ters of a large number of B-type stars in the Galactic, young ope
n cluster NGC 3293. The
determination of the stellar parameters is based on medium-
resolution spectra obtained with
FLAMES/GIRAFFE at ESO-VLT. As a second step, we adopted the acc
urate parameters to
determine the chemical abundances of these hot stars. We pre
sent a comparison of our results
with those obtained by the ’VLT-FLAMES survey of massive sta
rs’ (Evans et al. 2005). Our
study increases the number of objects analysed and provides an
extended view of this cluster.
