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Chasing the impact of the Gaia-Sausage-Enceladus merger on the formation of the Milky Way thick disc

Ciucă, I, Kawata, D, Ting, YS, Grand, RJJ, Miglio, A, Hayden, M, Baba, J, Fragkoudi, F, Monty, S, Buder, S and Freeman, K (2023) Chasing the impact of the Gaia-Sausage-Enceladus merger on the formation of the Milky Way thick disc. Monthly Notices of the Royal Astronomical Society: Letters, 528 (1). L122-L126. ISSN 1745-3925

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Abstract

We employ our Bayesian Machine Learning framework BINGO (Bayesian INference for Galactic archaeOlogy) to obtain high-quality stellar age estimates for 68 360 red giant and red clump stars present in the 17th data release of the Sloan Digital Sky Survey, the APOGEE-2 high-resolution spectroscopic survey. By examining the denoised age-metallicity relationship of the Galactic disc stars, we identify a drop in metallicity with an increase in [Mg/Fe] at an early epoch, followed by a chemical enrichment episode with increasing [Fe/H] and decreasing [Mg/Fe]. This result is congruent with the chemical evolution induced by an early-epoch gas-rich merger identified in the Milky Way-like zoom-in cosmological simulation Auriga. In the initial phase of the merger of Auriga 18 there is a drop in metallicity due to the merger diluting the metal content and an increase in the [Mg/Fe] of the primary galaxy. Our findings suggest that the last massive merger of our Galaxy, the Gaia-Sausage-Enceladus, was likely a significant gas-rich merger and induced a starburst, contributing to the chemical enrichment and building of the metal-rich part of the thick disc at an early epoch.

Item Type: Article
Uncontrolled Keywords: 0201 Astronomical and Space Sciences
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: Oxford University Press (OUP)
SWORD Depositor: A Symplectic
Date Deposited: 23 Sep 2024 15:58
Last Modified: 23 Sep 2024 16:00
DOI or ID number: 10.1093/mnrasl/slad033
URI: https://researchonline.ljmu.ac.uk/id/eprint/24242
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