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Lithium abundances in late main sequence stars. The case of the hyades
Published online by Cambridge University Press: 04 August 2017
Extract
It is well known that light elements like lithium are good indicators of the hydrodynamical behaviour of the outerlayers of the stars. As they are nuclearly destroyed at low temperature, i.e. close to the surface, their surface abundances reflect the nature of the transport process at work between the photosphere and the nuclear destruction region.
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- III. BINARITY, PULSATION, ROTATION AND MIXING
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- Copyright © Reidel 1984