000002720 001__ 2720
000002720 005__ 20160701171709.0
000002720 0247_ $$2DOI$$a10.1017/S1743921314006322
000002720 037__ $$aASTROimport-877
000002720 100__ $$aBlomme, R.
000002720 245__ $$aThe Gaia-ESO Survey and Massive Stars
000002720 260__ $$c2015
000002720 520__ $$aAs part of the Gaia-ESO Survey (GES), a number of clusters will be observed that were chosen specifically for their massive-star content. We report on the procedures we followed to determine the stellar parameters from the massive-star spectra of this survey. We intercompare the results from the different techniques used by the nodes of our group to determine these parameters and discuss some of the problems encountered. We present preliminary results for NGC 6705, NGC 3293, and Trumpler 14. We study microturbulence in A-type stars, we use the repeat observation to investigate binarity, and we determine cluster membership from the radial velocity information. The large number of massive-star spectra obtained by the Gaia-ESO Survey will allow us to critically test stellar evolution modelling. 
000002720 700__ $$a Frémat, Y.
000002720 700__ $$a Gosset, E.
000002720 700__ $$a Herrero, A.
000002720 700__ $$a Lobel, A.
000002720 700__ $$a Maíz Apellániz, J.
000002720 700__ $$a Morel, T.
000002720 700__ $$a Negueruela, I.
000002720 700__ $$a Semaan, T.
000002720 700__ $$a Simón-Díaz, S.
000002720 700__ $$a Volpi, D.
000002720 773__ $$c88-89$$pNew Windows on Massive Stars$$v307$$y2015
000002720 85642 $$ahttp://esoads.eso.org/abs/2015IAUS..307...88B
000002720 905__ $$apublished in
000002720 980__ $$aNONREF