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The Iron Abundances, [Fe/H] in the Four Nearest Open Clusters: Pleiades, Ursa Major Stream, Coma Berenices and Hyades
Published online by Cambridge University Press: 19 July 2016
Abstract
Iron abundances, [Fe/H] have been studied in G and K dwarfs of the four nearest clusters. With the exception of the Pleiades stars which are all fainter than the 10th magnitude, the observational material consists of high resolution, high S/N spectra taken at the coudé Reticon spectrograph of the Canada, France Hawaii Telescope. The Hyades is the only cluster with a significative overmetallicity with respect to the Sun.
- Type
- VI. Chemical Composition of Stars
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- Copyright © Kluwer 1988
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