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Title: Spatial variations in the Milky Way disc metallicity–age relation
ABSTRACT Stellar ages are a crucial component to studying the evolution of the Milky Way. Using Gaia DR2 distance estimates, it is now possible to estimate stellar ages for a larger volume of evolved stars through isochrone matching. This work presents [M/H]–age and [α/M]–age relations derived for different spatial locations in the Milky Way disc. These relations are derived by hierarchically modelling the star formation history of stars within a given chemical abundance bin. For the first time, we directly observe that significant variation is apparent in the [M/H]–age relation as a function of both Galactocentric radius and distance from the disc mid-plane. The [M/H]–age relations support claims that radial migration has a significant effect in the plane of the disc. Using the [M/H] bin with the youngest mean age at each radial zone in the plane of the disc, the present-day metallicity gradient is measured to be −0.059 ± 0.010 dex kpc−1, in agreement with Cepheids and young field stars. We find a vertically flared distribution of young stars in the outer disc, confirming predictions of models and previous observations. The mean age of the [M/H]–[α/M] distribution of the solar neighbourhood suggests that the high-[M/H] stars are not an evolutionary extension more » of the low-α sequence. Our observational results are important constraints to Galactic simulations and models of chemical evolution. « less
Authors:
; ; ; ; ; ; ;
Award ID(s):
1715662 1311835
Publication Date:
NSF-PAR ID:
10172184
Journal Name:
Monthly Notices of the Royal Astronomical Society
Volume:
489
Issue:
2
Page Range or eLocation-ID:
1742 to 1752
ISSN:
0035-8711
Sponsoring Org:
National Science Foundation
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