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Beryllium and Lithium Abundances in Stars with a Range of Metallicities
Published online by Cambridge University Press: 12 April 2016
Abstract
We present new beryllium abundances for three unevolved stars with [Fe/H] in the range −0.4 to −1.6. The Be II doublet is detected in the three stars. A spectral synthesis analysis has been conducted to derive the abundances. We briefly discuss their Be and Li abundances, together with a wide sample of stars from the literature, in the context of mixing processes below the convection zone.
- Type
- II. Atmospheres, a window to the interior
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- Copyright © Astronomical Society of the Pacific 1993