CORDIS Project
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This project focuses on globular clusters, studying very low mass stars and brown dwarfs to gain insights into early star formation in the Galaxy. It also examines blue stragglers to understand the dynamic evolution of these stellar systems.
Globular clusters (GCs) are the oldest stellar systems in the Galaxy and can be regarded as fossils from the violent epoch of Galaxy formation.
The lifetimes of their very low mass main sequence stars (VLMMSSs) and brown dwarfs (BDs) are much longer than the age of the Galaxy, and thus samples of the VLMMSSs and BDs in GCs can provide us with important insights into the earliest stages of star formation in the Galaxy.
Moreover, BDs represent a link between the lowest mass stars and giant planets…
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