000002750 001__ 2750
000002750 005__ 20160701171710.0
000002750 037__ $$aASTROimport-907
000002750 100__ $$aBlomme, R.
000002750 245__ $$aMassive Stars in the Gaia-ESO Survey
000002750 260__ $$c2013
000002750 520__ $$aThe Gaia-ESO Survey (GES) is an ambitious project to study the formation and evolution of the Milky Way and its stellar populations. It is led by Gerry Gilmore and Sofia Randich and includes about 350 Co-Investigators. During 300 nights (spread over 5 years) of order 10^5 Giraffe spectra and 10^4 UVES spectra will be taken. As part of the survey, about 13 clusters will be observed that were chosen specifically for their massive-star content. We report on the preliminary analysis of GES data from two such clusters: NGC 3293 and NGC 6705. We determine stellar parameters for the B-type stars in NGC 3293 and compare the A-type stars population between the two clusters. We also use a repeat observation to study binarity and use the radial velocity information to study cluster membership in NGC 3293. We also list our plans for future observations, which include the Carina nebula region. 
000002750 700__ $$a Fremat, Y.
000002750 700__ $$a Lobel, A.
000002750 700__ $$a Maíz Apellániz, J.
000002750 700__ $$a Morel, T.
000002750 700__ $$a Negueruela, I.
000002750 700__ $$a Semaan, T.
000002750 773__ $$c55$$pMassive Stars: From alpha to Omega$$y2013
000002750 85642 $$ahttp://esoads.eso.org/abs/2013msao.confE..55B
000002750 905__ $$apublished in
000002750 980__ $$aNONREF