Abstract.
Since the Galactic Open Clusters (OCs) provide a sample of stars
homogeneous in age and chemical composition and their distances are
well determined, they were recognized as suitable candidates to
study the chemical evolution of Galaxy. We have analyzed
high-dispersion echelle spectra (R≥50,000) of 3-4 red giant
members for each open cluster to derive abundances for a whole range
of elements including light as well as heavy elements. The
membership to the cluster has been confirmed through their radial
velocities and proper motions. The spread in temperatures and
gravities being very small, nearly the same stellar lines were
employed thereby reducing the random errors. Most of these clusters
are located in Galactic anti-center direction and we found [Fe/H]
values of -0.02$±$0.05 for NGC 752, -0.07$±0.06 for NGC
2360, -0.11±0.05 for NGC 1817 and -0.19±0.06 for NGC
2506. Abundances relative to Fe for elements from Na to Eu are equal
within measurement uncertainties to published abundances for thin
disk giants in the field with the possible exception of mild
anomalies for Mn, Cu, Ba, Ce and Nd. This supports the view that
field stars come from disrupted open clusters.
Key words: Galaxy: abundances -- stars: abundances