1999/12/07 by A. Bragaglia, M. Tosi, Bragaglia, A. +5
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9912130
6 pages, 3 figures, to appear in "The chemical evolution of the Milky Way: Stars versus clusters", September 20-24, Vulcano
arxiv created 1999/12/07 · arxiv updated 2009/12/01
Old open clusters are useful tools to study the Galactic disk properties, both present and past. Populous samples with properties determined both accurately and homogenously are necessary to draw reliable conclusions. We present here our recent work in the field and introduce and discuss results on metallicities.