Constraints on the Frequency and Mass Content of r-process Events Derived from Turbulent Mixing in Galactic Disks

Constraints on the Frequency and Mass Content of r-process Events Derived from Turbulent Mixing in Galactic Disks

Metal-poor stars in the Milky Way (MW) halo display large star-to-star dispersion in their r -process abundance relative to lighter elements. This suggests a chemically diverse and unmixed interstellar medium (ISM) in the early universe. This study aims to help shed light on the impact of turbulent...

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Bibliographic Details
Main Authors: Anne Noer Kolborg, Enrico Ramirez-Ruiz, Davide Martizzi, Phillip Macias, Melinda Soares-Furtado
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
R-process
Stellar feedback
Metallicity
Interstellar medium
Galactic winds
Milky Way Galaxy physics
Online Access:https://doi.org/10.3847/1538-4357/acca80

Internet

https://doi.org/10.3847/1538-4357/acca80

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