The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved H i maps

ABSTRACT Cold gas in galaxies provides a crucial test to evaluate the realism of cosmological hydrodynamical simulations. To extract the atomic and molecular hydrogen properties of the simulated galaxy population, post-processing methods taking the local UV field into account are required. We improv...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2023-03, Vol.521 (4), p.5645-5668
Hauptverfasser:	Gebek, Andrea, Baes, Maarten, Diemer, Benedikt, de Blok, W J G, Nelson, Dylan, Kapoor, Anand Utsav, Camps, Peter, Rabyang, Omphile, Leeuw, Lerothodi
Format:	Artikel
Sprache:	eng
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