Title
VizieR Online Data Catalog: S abundances for 1301 stars from GES (Duffau+, 2017)
Journal
VizieR Online Data Catalog
Date Issued
2017
Author(s)
Duffau, S.
Caffau, E.
Sbordone, L.
Bonifacio, P.
Andrievsky, S.
Korotin, S.
Babusiaux, C.
Salvadori, S.
Monaco, L.
Francois, P.
Skuladottir, A.
Spina, L.
Gallagher, A. J.
Ludwig, H. -G.
Christlieb, N.
Hansen, C. J.
Mott, A.
Steffen, M.
Blanco-Cuaresma, S.
Friel, E.
Jimenez-Esteban, F. M.
Koch, A.
Tang, B.
Tautvaisiene, G.
Hawkins, K.
Gilmore, G.
Feltzing, S.
Bensby, T.
Smiljanic, R.
Bayo, A.
Carraro, G.
Casey, A. R.
Costado, M. T.
Hourihane, A.
Jofre, P.
Lardo, C.
Lewis, J.
Sousa, S. G.
Worley, C. C.
DOI
10.26093/cds/vizier.36040128
Abstract
GES internal star identifier (CNAME), Sulphur abundances and NLTE corrections to the Sulphur abundances for 1301 stars. Sulphur abundances are expressed in the customary logarithmic form: A(S)=log_10(N(S)/N(H))+12. The abundances delivered are the LTE ones. NLTEabundances can be determined by directly summing the NLTE correction delivered: A(S)<SUB>NLTE = A(S) + NLTE</SUB>C. So that a negative NLTE correction indicates that the NLTE abundance is lower than the LTE one. (1 data file).
File(s)