We present the results of the analysis of an extensive set of new and literature high quality data concerning Fe, C, N, O, Na, and Mg. This analysis exploited the T_eff_ scale determined in Gratton et al. (1996, Cat. ), and the non-LTE abundance corrections computed in Gratton et al. (1999, Cat. ). Results obtained with various abundance indices are discussed and compared.
Cone search capability for table J/A+A/356/238/table2 (Equivalent widths for O, Na lines in the 19 program stars and the Sun)