All Tables

• Table 1: Atomic data of Na lines. values and damping constants have been determined from solar spectrum fits.
• Table 2: Atmospheric parameters and sodium abundances of the program stars. Rotational velocities and macroturbulence data are the same as in Fuhrmann (1998, 2000).
• Table 3: Abundance differences between NLTE and LTE obtained by fitting calculated LTE equivalent widths of Na I lines using the same parameters for various stellar model atmospheres based on the line-blanketed model grid. Results refer to [Na/Fe] . No entries are given for extremely weak lines. The calculations all refer to km s^-1 and [Na/Fe] = 0.