Exploring the Chemical Fingerprints of Metal-Poor Stars: Insights from the MINCE III Project

The MINCE III project analyzes 99 intermediate-metallicity stars to understand neutron-capture elements, key to the Milky Way’s chemical history. Using high-resolution spectra, the study reveals chemical abundances, including unique findings like a lithium-rich star. Results align with models of Galactic evolution, highlighting the origins of heavy elements through processes like supernovae and neutron-star mergers, advancing our understanding of the Galaxy's formation.