CORDIS Project
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This project focuses on analyzing the local stellar population within 100 parsecs of the Sun using medium resolution optical spectroscopy. By studying stars and white dwarfs, it aims to enhance our understanding of stellar evolution and the formation history of the Milky Way.
The stellar population near the Sun, which contains the brightest specimens of almost all types of stars and planets, is a key research area that remains poorly explored.
The spacecraft Gaia has provided, for the first time, a near complete census of stars and white dwarfs within 100 pc, but a full understanding of the local stellar population is still a major challenge.
From this project and my involvement in the next generation multi-object spectroscopic surveys 4MOST and WEAVE, I will obtain…
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