CORDIS Project
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This project focuses on improving models of the Thermally Pulsing Asymptotic Giant Branch stars to enhance our understanding of stellar evolution and its implications for galaxy formation. It combines theoretical modeling with high-quality observational data to resolve existing uncertainties.
Models of the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) stellar evolutionary phase play a critical role across astrophysics, from the chemical composition of meteorites belonging to the pre-solar nebula up to galaxy evolution in the high-redshift Universe.
In spite of its importance, the modelling of TP-AGB is still affected by large uncertainties that propagate into the field of extragalactic astronomy, degrading the predicting power of current population synthesis models of galaxies.…
UNIVERSITA DEGLI STUDI DI PADOVA
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