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Gaia-ESO survey: the analysis of pre-main sequence stellar spectra

Lanzafame, A. C; Frasca, A; Damiani, F; Franciosini, E; Cottaar, M; Sousa, S. G; Tabernero, H. M; Klutsch, A; Spina, L; Biazzo, K; Prisinzano, L; Sacco, G. G.; Randich, S; Brugaletta, E; Delgado Mena, E; Adibekyan, V; Montes, D; Bonito, R; Gameiro, J. F; Alcalá, J. M; González Hernández, J. I; Jeffries, R; Messina, S; Meyer, M; Gilmore, G; Asplund, M; Binney, J.; Bonifacio, P.; Drew, J. E.; Feltzing, S.; Ferguson, A. M. N.; Micela, G.; Negueruela, I.; Prusti, T.; Rix, H-W.; Vallenari, A.; Alfaro, E. J.; Allende Prieto, C.; Babusiaux, C.; Bensby, T.; Blomme, R.; Bragaglia, A.; Flaccomio, E.; Francois, P.; Hambly, N.; Irwin, M.; Koposov, S. E.; Korn, A. J.; Smiljanic, R.; Van Eck, S.; Walton, N.; Bayo, A.; Bergemann, M.; Carraro, G.; Costado, M. T.; Edvardsson, B.; Heiter, U.; Hill, V.; Hourihane, A.; Jackson, R. J.; Jofré, P.; Lardo, C.; Lewis, J.; Lind, K.; Magrini, L.; Marconi, G.; Martayan, C.; Masseron, T.; Monaco, L.; Morbidelli, L.; Sbordone, L.; Worley, C. C.; Zaggia, S.

Description

This paper describes the analysis of UVES and GIRAFFE spectra acquired by the Gaia-ESO Public Spectroscopic Survey in the fields of young clusters whose population includes pre-main sequence (PMS) stars. Both methods that have been extensively used in the past and new ones developed in the contest of the Gaia-ESO survey enterprise are available and used. The internal precision of these quantities is estimated by inter-comparing the results obtained by such different methods, while the...[Show more]

CollectionsANU Research Publications
Date published: 2015-01-19
Type: Journal article
URI: http://hdl.handle.net/1885/14217
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201424759

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