All Tables

Table 1: Parameters of the program stars. The data were taken from the Bright Star Catalogue (Hoffleit & Warren 1991). Distances have been calculated using HIPPARCOS parallaxes (ESA 1997). The last column indicates whether a star was observed from ESO (E) or SAO (S).
Table 2: This table comprises all lines used for the abundance analysis. In Cols. 3 and 4 we compiled the contributions of blend lines and additional comments, respectively.
Table 3: Energy levels of the O I model atom.
Table 4: Line transitions of the O I model atom: Lower level number (Low), upper level number (Up), wavelength and $\log gf$ -value (Wiese et al. 1996).
Table 5: LTE and NLTE abundances. The NLTE corrections and abundances of C, O and Ne are given with respect to the solar values.
Table 6: LTE and NLTE abundances. The NLTE corrections and abundances of Mg, Si and Ca are given with respect to the solar values.
Table 7: LTE and NLTE abundances. The NLTE corrections and abundances of Fe, Sr and Ba are given with respect to the solar values.
Table 8: Equivalent widths of the detected narrow absorption features.