The Gaia-ESO Survey and Massive Stars

Bibcode
2015IAUS..307...88B
DOI
10.1017/S1743921314006322
Blomme, R.; Frémat, Yves; Gosset, Eric; Herrero, A.; Lobel, Alex; Apellániz, Jesús Maíz; Morel, Thierry; Negueruela, Ignacio; Semaan, Thierry; Simón-Díaz, Sergio; Volpi, Delia
Bibliographical reference

New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry, Proceedings of the International Astronomical Union, IAU Symposium, Volume 307, pp. 88-89

Advertised on:
1
2015
Number of authors
11
IAC number of authors
2
Citations
1
Refereed citations
1
Description
As 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.
Type
Non-refereed
Surveys

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