The origin of the $\alpha$-enhancement of massive galaxies
Marijke C. Segers, Joop Schaye, Richard G. Bower, Robert A. Crain,, Matthieu Schaller, Tom Theuns

TL;DR
This study uses cosmological simulations to explore how active galactic nucleus feedback influences the alpha-element enhancement in massive galaxies, aligning with observed trends and supporting a downsizing formation scenario.
Contribution
It demonstrates that AGN feedback is crucial in explaining the alpha-enhancement in massive galaxies by quenching star formation early, which was not fully understood before.
Findings
AGN feedback suppresses star formation in massive galaxies
Alpha-enhancement correlates with galaxy mass and age
Without AGN, alpha-enhancement trends differ significantly
Abstract
We study the origin of the stellar -element-to-iron abundance ratio, , of present-day central galaxies, using cosmological, hydrodynamical simulations from the Evolution and Assembly of GaLaxies and their Environments (EAGLE) project. For galaxies with stellar masses of M, increases with increasing galaxy stellar mass and age. These trends are in good agreement with observations of early-type galaxies, and are consistent with a `downsizing' galaxy formation scenario: more massive galaxies have formed the bulk of their stars earlier and more rapidly, hence from an interstellar medium that was mostly -enriched by massive stars. In the absence of feedback from active galactic nuclei (AGN), however, in M galaxies is…
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