The Relationship between Age, Metallicity, and Abundances for Disk Stars in a Simulated Milky Way
Observations of the Milky Way’s low- α disk show that several element abundances correlate with age at fixed metallicity, with unique slopes and small scatters around the age–[X/Fe] relations. In this study, we turn to simulations to explore the age–[X/Fe] relations for the elements C, N, O, Mg, Si,...
Hlavní autoři: | , , , , , , |
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Médium: | Článek |
Jazyk: | English |
Vydáno: |
IOP Publishing
2023-01-01
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Edice: | The Astrophysical Journal |
Témata: | |
On-line přístup: | https://doi.org/10.3847/1538-4357/aca1c7 |