000002718 001__ 2718
000002718 005__ 20160701171709.0
000002718 0247_ $$2DOI$$a10.1017/S1743921314006577
000002718 037__ $$aASTROimport-875
000002718 100__ $$aSemaan, T.
000002718 245__ $$aNGC 3293 revisited by the Gaia-ESO Survey
000002718 260__ $$c2015
000002718 520__ $$aIn the framework of the Gaia-ESO survey we have determined the fundamental parameters of a large number of B-type stars in the Galactic, young open cluster NGC 3293. The determination of the stellar parameters is based on medium-resolution spectra obtained with FLAMES/GIRAFFE at ESO-VLT. As a second step, we adopted the accurate parameters to determine the chemical abundances of these hot stars. We present a comparison of our results with those obtained by the 'VLT-FLAMES survey of massive stars' (Evans et al. 2005). Our study increases the number of objects analysed and provides an extended view of this cluster. 
000002718 700__ $$a Morel, T.
000002718 700__ $$a Gosset, E.
000002718 700__ $$a Zorec, J.
000002718 700__ $$a Frémat, Y.
000002718 700__ $$a Blomme, R.
000002718 700__ $$a Lobel, A.
000002718 773__ $$c140-141$$pNew Windows on Massive Stars$$v307$$y2015
000002718 85642 $$ahttp://esoads.eso.org/abs/2015IAUS..307..140S
000002718 905__ $$apublished in
000002718 980__ $$aNONREF