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Abundances of Light Metals in Field Stars with Metallicity Range −1.2 < [Fe/H] < + 0.3
Published online by Cambridge University Press: 19 July 2016
Abstract
High resolution, high S:N spectra are used to determine the abundances of Fe, Ni, Ca, Al and Si in 25 field dwarfs with −1.2<[Fe/H]< +0.3. We find overabundances for Al, Ca and Si in stars with −1.2<[Fe/H]< −0.5 and solar [Ni/Fe] over the whole studied range.
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- VI. Chemical Composition of Stars
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- Copyright © Kluwer 1988