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,...

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Hlavní autoři: Andreia Carrillo, Melissa K. Ness, Keith Hawkins, Robyn E. Sanderson, Kaile Wang, Andrew Wetzel, Matthew A. Bellardini
Médium: Článek
Jazyk:English
Vydáno: IOP Publishing 2023-01-01
Edice:The Astrophysical Journal
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On-line přístup:https://doi.org/10.3847/1538-4357/aca1c7