Abstract

We have measured the abundances of Fe, Si, Ni, Ti, and Na in 20 Pleiads with \teff values near solar and with low \vsini using high-resolution, high signal-to-noise echelle spectra. We have validated our procedures by also analyzing 10 field stars of a range of temperatures and metallicities that were observed by \citet{Vale05}. Our result for the Pleiades is [Fe/H] = +0.03±0.02±0.05+0.03\pm0.02\pm0.05 (statistical and systematic). The average of published measurements for the Pleiades is +0.042±0.021+0.042\pm0.021.

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