Clues to the formation of the Milky Way's thick disk
M. Haywood, P. Di Matteo, O. Snaith, M. Lehnert

TL;DR
This study investigates the chemical properties of stars in the Milky Way's thick disk, suggesting a uniform star formation history and a pre-assembled gas disk, challenging inside-out formation models.
Contribution
It provides evidence that the thick disk's formation was likely a rapid, pre-assembled process with minimal inside-out growth, contrasting with traditional models.
Findings
Small dispersion in alpha-element abundances across ages.
Lack of radial metallicity gradient in the thick disk.
Evidence for a pre-assembled, closed-box like early disk.
Abstract
We analyse the chemical properties of a set of solar vicinity stars, and show that the small dispersion in abundances of \alpha-elements at all ages provides evidence that the SFH has been uniform throughout the thick disk. In the context of long time scale infall models, we suggest that this result points either to a limited dependence of the gas accretion on the Galactic radius in the inner disk (R<10 kpc), or to a decoupling of the accretion history and star formation history due to other processes governing the ISM in the early disk, suggesting that infall cannot be a determining parameter of the chemical evolution at these epochs. We argue however that these results and other recent observational constraints -- namely the lack of radial metallicity gradient and the non-evolving scale length of the thick disk -- are better explained if the early disk is viewed as a pre-assembled…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
