  Europium abundances for 74 F and G dwarf stars of the galactic disk have been
determined from the 4129.7 A Eu II line. The stars were selected from the
sample of Edvardsson et al. (1993) and [Eu/Fe] shows a smaller scatter and a
slightly weaker trend with [Fe/H] than found by Woolf et al. (1995). The data
of the two analyses are homogenized and merged. We also discuss the adopted
effective temperature scale.
