Stellar lithium abundances may not be representative of the interstellar medium composition. The study: “The Gaia-ESO Survey: Probing the lithium abundances in old metal-rich dwarf stars in the solar vicinity” of M. L. L. Dantas (Nicolaus Copernicus Astronomical Center) appeared on A&A

The study of chemical abundances in the interstellar medium and stars in our Galaxy is of utmost importance, as it provides insights into the chemical enrichment of the galactic interstellar medium by massive stars and the evolution of different components of the Milky Way. Lithium is frequently the subject of spectroscopic surveys and studies aimed at determining its abundance in

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A catalog of Lithium abundances from the Gaia-ESO Survey. The study: “The Gaia-ESO Survey: Lithium measurements and new curves of growth” of E.Franciosini (INAF-OA Arcetri) recently appeared on A&A

In astrophysics, there are elements that provide important diagnostics used in various fields, such as Lithium. For instance, measurements of Lithium abundances are important in cosmology where there is a well-known problem of matching the measured abundances in population II stars with those predicted by cosmological models of Big Bang synthesis. Measurements of Lithium abundances are also essential for understanding

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Lithium abundance and stellar internal structure. The study: “The Gaia-ESO survey: Mixing processes in low-mass stars traced by lithium abundance in cluster and field stars” of L. Magrini (INAF – OA Arcetri) recently appeared on A&A

The chemical history of Lithium abundance in the Universe is very complex. This chemical element has been first produced during the Big Bang, even if in very small quantities compared with hydrogen and helium. Since then, lithium is continuously created and destroyed by several processes occurring in stellar interior. This means that the lithium abundances we observe in stars today

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