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S. Schuler, J. R. King (University of Nevada Las Vegas), D. A. Fischer (University of California at Berkeley), D. R. Soderblom (Space Telescope Science Institute)
Abundances of numerous elements are derived for several solar-type dwarfs in the young open cluster M34 from high-resolution (R~45,000) Keck/HIRES spectra. Results are presented and discussed to address their implications for intra-cluster abundance scatter, Galactic chemical evolution, and stellar Li depletion. This work was supported by NSF grant AST-0086576 to JRK.