Milky Way Mapper decoded abundances -- II: From patterns to paths
Melissa K. Ness, Sarah Aquilina, Jennifer Mead, Emily Griffith, Catherine Manea, Jonathan Bird, Andrew R. Casey, Lucy (Yuxi) Lu, Kathryn V. Johnston, Michael R. Blanton, James W. Johnson, Maja Jablonska, Leticia Carigi, Jos\'e G. Fern\'andez-Trincado, Ricardo L\'opez Valdivia

TL;DR
This study re-projects stellar abundances into shared enrichment patterns to uncover the Milky Way disc's chemical evolution, revealing low-dimensional structures linked to spatial, temporal, and dynamical processes.
Contribution
It introduces a generative framework that identifies coherent enrichment pathways and low-dimensional chemical structures in the Milky Way disc.
Findings
Reveals a low-dimensional enrichment basis responding to global disc evolution drivers.
Identifies enrichment pathways correlated with age, height, and radial position.
Discovers a transition at ~6 Gyr to a more chemically mixed regime.
Abstract
The element abundances of Milky Way disc stars encode entangled imprints of multiple enrichment processes, making it difficult to uncover the underlying chemical evolution. Here we re-project 16 stellar abundances for 199,290 red giant stars ([Fe/H]) into a set of (4) shared enrichment patterns, providing a generative framework for learning the organising structure of the Milky Way disc. The relative contributions of these patterns vary systematically across the disc, revealing a low-dimensional enrichment basis that responds coherently to global drivers of disc evolution. By grouping stars according to their pattern contributions, we identify coherent enrichment pathways that exhibit strong chemo-spatial correlations and are stratified in both age and height above the plane, linking radial growth to vertical disc structure. Stars occupying similar positions along these…
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