OCCASO - II. Physical parameters and Fe abundances of red clump stars in 18 open clusters
Open clusters have long been used to study the chemodynamical evolution of the Galactic disc. This requires a homogeneously analysed sample covering a wide range of ages and distances. In this paper, we present the Open Clusters Chemical Abundances from Spanish Observatories (OCCASO) second data release. This comprises a sample of high-resolution
Casamiquela, L. et al.
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10
2017