Description
We present parameter and abundance data for a sample of 298 nearby giants. The spectroscopic data for this work have a resolution of R~60000S/N>150, and spectral coverage from 475 to 685nm. Overall trends in the Z>10 abundances are dominated by Galactic chemical evolution, while the light-element abundances are influenced by stellar evolution, as well as Galactic evolution. We find several super-Li stars in our sample and confirm that Li abundances in the first giant branch are related to mixing depths.
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