Volume 381, Number 2, JanuaryII 2002
|Page(s)||500 - 506|
|Section||Stellar structure and evolution|
|Published online||15 January 2002|
Uppsala Astronomical Observatory, Box 515, 751 20 Uppsala, Sweden
Corresponding author: B. Edvardsson, Bengt.Edvardsson@astro.uu.se
Accepted: 15 October 2001
Europium abundances for 74 F and G dwarf stars of the galactic disk have been determined from the 4129.7 Å 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.
Key words: stars: abundances / Galaxy: abundances
© ESO, 2002
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