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A High S/N Spectroscopic Survey of Chemical Abundances in Disk Population F0-G2 Dwarfs
Published online by Cambridge University Press: 19 July 2016
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In collaboration with D. Lambert and J. Tomkin high resolution, high S/N spectra have been obtained for about 250 disk population F0-G2 dwarfs. The aim of this large programme is to study various abundance ratios as a function of [Fe/H] and stellar age. A detailed description of the project and some preliminary results were given by Nissen et al. (1985).
- Type
- VI. Chemical Composition of Stars
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- Copyright © Kluwer 1988
References
Nissen, P.E., Edvardsson, B., Gustafsson, B., Proc. ESO workshop on “Production and Distribution of C,N,O Elements”, Eds. Danziger, E. J., Matteucci, F. and Kjär, K., p.131.Google Scholar