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Open clusters as key tracers of Galactic chemical evolution III. Element abundances in Berkeley 20, Berkeley 29, Collinder 261, and Melotte 66SESTITO, P; BRAGAGLIA, A; RANDICH, S et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 488, Num 3, pp 943-958, issn 0004-6361, 16 p.Article
