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NGC 3293 revisited by the Gaia-ESO Survey

Published online by Cambridge University Press:  23 January 2015

Thierry Semaan
Affiliation:
ULg, Institut d'Astrophysique et de Géophysique, Liège, Belgium email: thierry.semaan@ulg.ac.be
Thierry Morel
Affiliation:
ULg, Institut d'Astrophysique et de Géophysique, Liège, Belgium email: thierry.semaan@ulg.ac.be
Eric Gosset
Affiliation:
ULg, Institut d'Astrophysique et de Géophysique, Liège, Belgium email: thierry.semaan@ulg.ac.be
Juan Zorec
Affiliation:
Institut d'Astrophysique de Paris, CNRS (UMR 7095), Paris, France & Université Pierre et Marie Curie (UMR 7095), Paris, France
Yves Frémat
Affiliation:
Royal Observatory of Belgium, Brussels, Belgium
Ronny Blomme
Affiliation:
Royal Observatory of Belgium, Brussels, Belgium
Alex Lobel
Affiliation:
Royal Observatory of Belgium, Brussels, Belgium
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Abstract

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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Asplund, M., Grevesse, N., Sauval, A. J., & Scott, P. 2009, ARA&A 47, 481Google Scholar
Evans, C. J., Smartt, S. J., Lee, J.-K., et al. 2005, A&A 437, 467Google Scholar
Frémat, Y., Neiner, C., Hubert, A.-M., et al. 2006, A&A 451, 1053Google Scholar
Hunter, I., Brott, I., Langer, N., et al. 2009, A&A 496, 841Google Scholar