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,...
Main Authors: | Andreia Carrillo, Melissa K. Ness, Keith Hawkins, Robyn E. Sanderson, Kaile Wang, Andrew Wetzel, Matthew A. Bellardini |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/aca1c7 |
Similar Items
-
The Chemical Enrichment of the Milky Way Disk Evaluated Using Conditional Abundances
by: Bridget L. Ratcliffe, et al.
Published: (2023-01-01) -
Chemodynamical Analysis of Metal-rich High-eccentricity Stars in the Milky Way's Disk
by: Ayeon Lee, et al.
Published: (2023-01-01) -
Icarus Revisited: An Ancient, Metal-poor Accreted Stellar Stream in the Disk of the Milky Way
by: Paola Re Fiorentin, et al.
Published: (2024-01-01) -
HALO7D. III. Chemical Abundances of Milky Way Halo Stars from Medium-resolution Spectra
by: Kevin A. McKinnon, et al.
Published: (2023-01-01) -
The Milky Way’s Rowdy Neighbors: The Effects of the Large Magellanic Cloud and Sagittarius Dwarf on the Milky Way Disk
by: Ioana A. Stelea, et al.
Published: (2024-01-01)