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

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...

Full description

Bibliographic Details
Main Authors: Stevens, Adam RH, Lagos, Claudia del P, Cortese, Luca, Catinella, Barbara, Diemer, Benedikt, Nelson, Dylan, Pillepich, Annalisa, Hernquist, Lars, Marinacci, Federico, Vogelsberger, Mark
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: Oxford University Press (OUP) 2022
Online Access:https://hdl.handle.net/1721.1/142399

Similar Items

Similar Items