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- W3033589769 abstract "Abstract Solar twins are stars with a mass and chemical composition similar to the Sun; therefore, they follow about the same evolution and can be used to study the past and future of the Sun. I review the evolution of lithium and beryllium in solar‐mass solar‐metallicity main sequence stars, using a differential spectroscopic analysis of solar twins relative to the Sun, allowing precise determination of stellar ages thanks to the precise stellar parameters ( T eff , log g , [Fe/H]) achieved with high‐resolution high S / N spectra. There is a clear trend of lithium depletion with increasing ages, while beryllium is only slightly depleted, suggesting a relatively shallow extra‐mixing in Sun‐like stars. I also discuss the possible connection between lithium and planets. Finally, I review lithium and beryllium in binary solar analogs with mass‐transfer events (“blue lurkers”)." @default.
- W3033589769 created "2020-06-12" @default.
- W3033589769 creator A5054681294 @default.
- W3033589769 date "2020-06-01" @default.
- W3033589769 modified "2023-09-24" @default.
- W3033589769 title "Lithium and beryllium in solar twins" @default.
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- W3033589769 doi "https://doi.org/10.1002/asna.202013755" @default.
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