2718 20160701171709.0 10.1017/S1743921314006577 DOI ASTROimport-875 Semaan, T. 2015 NGC 3293 revisited by the Gaia-ESO Survey In the framework of the Gaia-ESO survey we have determined the fundamental parameters of a large number of B-type stars in the Galactic, young open 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 accurate parameters to determine the chemical abundances of these hot stars. We present a comparison of our results with those obtained by the 'VLT-FLAMES survey of massive stars' (Evans et al. 2005). Our study increases the number of objects analysed and provides an extended view of this cluster. Morel, T. Gosset, E. Zorec, J. Frémat, Y. Blomme, R. Lobel, A. New Windows on Massive Stars 307 2015 140-141 http://esoads.eso.org/abs/2015IAUS..307..140S published in NONREF