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The growth of a lithium abundance dispersion in pre-main-sequence stars (2025)
Journal Article
Jackson, R. J., Jeffries, R. D., & Tognelli, E. (2025). The growth of a lithium abundance dispersion in pre-main-sequence stars. Monthly Notices of the Royal Astronomical Society, 539(4), 3364-3380. https://doi.org/10.1093/mnras/staf683

Lithium is predicted, and observed, to be depleted in contracting low-mass pre-main-sequence (PMS) stars. Yet, these stars reach the zero-age main-sequence (ZAMS) with a spread in lithium abundance at a given effective temperature that is not predict... Read More about The growth of a lithium abundance dispersion in pre-main-sequence stars.

The Gaia-ESO Survey: Homogenisation of stellar parameters and elemental abundances (2023)
Journal Article
Hourihane, A., François, P., Worley, C. C., Magrini, L., Gonneau, A., Casey, A. R., Gilmore, G., Randich, S., Sacco, G. G., Recio-Blanco, A., Korn, A. J., Allende Prieto, C., Smiljanic, R., Blomme, R., Bragaglia, A., Walton, N. A., Van Eck, S., Bensby, T., Lanzafame, A., Frasca, A., …Minkevičiūtė, R. (2023). The Gaia-ESO Survey: Homogenisation of stellar parameters and elemental abundances. Astronomy & Astrophysics, 676, Article A129. https://doi.org/10.1051/0004-6361/202345910

The Gaia-ESO Survey is a public spectroscopic survey that targeted greater than or similar to 10(5) stars covering all major components of the Milky Way from the end of 2011 to 2018, delivering its final public release in May 2022. Unlike other spect... Read More about The Gaia-ESO Survey: Homogenisation of stellar parameters and elemental abundances.