Open clusters as key tracers of Galactic chemical evolution - III. Element abundances in Berkeley 20, Berkeley 29, Collinder 261, and Melotte 66
A&A, 488 3 (2008) 943-958
Published online: 2008-07-09
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CNONa and ${^{12}}$C/${^{13}}$C in giant stars of 10 open clusters
R. Smiljanic, R. Gauderon, P. North, et al.Astronomy & Astrophysics 502 (1) 267 (2009)
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Metallicity gradients in the Milky Way
Walter J. Maciel and Roberto D. D. CostaProceedings of the International Astronomical Union 5 (S265) 317 (2009)
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ENHANCED PRODUCTION OF BARIUM IN LOW-MASS STARS: EVIDENCE FROM OPEN CLUSTERS
Valentina D'Orazi, Laura Magrini, Sofia Randich, et al.The Astrophysical Journal 693 (1) L31 (2009)
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The evolution of the Galactic metallicity gradient from high-resolution spectroscopy of open clusters
L. Magrini, P. Sestito, S. Randich and D. GalliAstronomy & Astrophysics 494 (1) 95 (2009)
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Chemical composition of the young open clusters IC 2602 and IC 2391
V. D'Orazi and S. RandichAstronomy & Astrophysics 501 (2) 553 (2009)
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The Bologna Open Cluster Chemical Evolution project: a large, homogeneous sample of Galactic open clusters
Angela BragagliaProceedings of the International Astronomical Union 4 (S258) 153 (2008)
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