2023
DOI: 10.1093/mnras/stad1587
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The relationship between cluster environment and molecular gas content of star-forming galaxies in the eagle simulation

Abstract: We employ the eagle hydrodynamical simulation to uncover the relationship between cluster environment and H2 content of star-forming galaxies at redshifts spanning 0 ≤ z ≤ 1. To do so, we divide the star-forming sample into those that are bound to clusters and those that are not. We find that, at any given redshift, the galaxies in clusters generally have less H2 than their non-cluster counterparts with the same stellar mass (corresponding to an offset of ≲ 0.5 dex), but this offset varies with stellar mass an… Show more

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