Abstract
We report on the status of an observational program aimed at determining the lithium abundance in a large volume-limited sample of nearby solar-type (with spectral-types ranging from late-F to late-K) stars. Although the results presented here are preliminary, in that the data reduction is not completed yet, the sample is already large enough to be reasonably representative of the “typical” behavior of normal stars in this mass range.
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© 1995 Springer-Verlag Berlin Heidelberg
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Favata, F., Micela, G., Sciortino, S. (1995). Lithium in Nearby Main-Sequence Solar-Type Stars. In: Crane, P. (eds) The Light Element Abundances. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49169-9_41
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DOI: https://doi.org/10.1007/978-3-540-49169-9_41
Publisher Name: Springer, Berlin, Heidelberg
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