Observations of Li-rich giant stars in the Galaxy and in the Magellanic Clouds
The Lithium content in stars is very sensitive to the internal stellar conditions. Indeed, Lithium is readily destroyed in the interiors of low-mass main-sequence (MS) stars and the Li in the convective envelope is progressively depleted. The Li abundance at the stellar surface was expected to be further depleted after stars leave the MS and
García-Hernández, D. A.
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2020