Topics on Galactic Chemical Evolution
Nikos Prantzos (UPMC, Institut d'Astrophysique de Paris)

TL;DR
This paper explores key issues in Galactic chemical evolution, including the absence of secondary element signatures, halo formation through hierarchical models, and the impact of radial migration on disk evolution.
Contribution
It provides a comprehensive discussion on three distinct topics, integrating observational data and recent theoretical developments in Galactic evolution.
Findings
No observational signature of secondary elements detected
Galactic halo likely formed via hierarchical galaxy formation
Radial migration significantly influences disk evolution
Abstract
I discuss three different topics in Galactic chemical evolution:the "puzzling" absence of any observational signature of secondary elements ; the building of the Galactic halo in the framework of hierarchical galaxy formation, as evidenced from its metallicity distribution ; and the potentially important role that radial migration may play in the evolution of galactic disks, according to recent studies.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · SAS software applications and methods
