Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO and SFR data

We examine how the post-processed content of molecular hydrogen (H2) in galaxies from the TNG100 cosmological, hydrodynamic simulation changes with environment at z = 0, assessing central/satellite status and host halo mass. We make close comparisons with the carbon monoxide (CO) emission survey xCO...

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Bibliographic Details
Main Authors: Stevens, Adam RH (Author), Lagos, Claudia del P (Author), Cortese, Luca (Author), Catinella, Barbara (Author), Diemer, Benedikt (Author), Nelson, Dylan (Author), Pillepich, Annalisa (Author), Hernquist, Lars (Author), Marinacci, Federico (Author), Vogelsberger, Mark (Author)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2022-05-06T16:38:47Z.
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