Titolo: | VizieR Online Data Catalog: S abundances for 1301 stars from GES (Duffau+, 2017) |
Autori: | Duffau, S. Caffau, E. Sbordone, L. Bonifacio, P. Andrievsky, S. Korotin, S. Babusiaux, C. Salvadori, S. Monaco, L. Francois, P. Skuladottir, A. BRAGAGLIA, Angela Donati, P. Spina, L. Gallagher, A. J. Ludwig, H. -G. Christlieb, N. Hansen, C. J. Mott, A. Steffen, M. ZAGGIA, Simone Blanco-Cuaresma, S. Calura, F. Friel, E. Jimenez-Esteban, F. M. Koch, A. MAGRINI, LAURA PANCINO, ELENA Tang, B. Tautvaisiene, G. VALLENARI, Antonella Hawkins, K. Gilmore, G. RANDICH, Maria Sofia Feltzing, S. Bensby, T. FLACCOMIO, Ettore Smiljanic, R. Bayo, A. Carraro, G. Casey, A. R. Costado, M. T. DAMIANI, Francesco FRANCIOSINI, Elena Hourihane, A. Jofre, P. Lardo, C. Lewis, J. Morbidelli, L. Sousa, S. G. Worley, C. C. |
Data pubblicazione: | 2017 |
Rivista: | VizieR Online Data Catalog |
Da pagina:: | J/A+A/604/A128 |
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). |
URI: | http://hdl.handle.net/20.500.12386/26715 |
URL: | http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/604/A128 |
DOI: | 10.26093/cds/vizier.36040128 |
Bibcode ADS: | 2017yCat..36040128D |
Fulltext: | open |
È visualizzato nelle collezioni: | 4.06 Banche Dati
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