Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations

Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations

We compare the star-forming main sequence (SFMS) of galaxies - both integrated and resolved on 1 kpc scales - between the high-resolution TNG50 simulation of IllustrisTNG and observations from the 3D-HST slitless spectroscopic survey at z ∼ 1. Contrasting integrated star formation rates (SFRs), we f...

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Bibliographic Details
Main Authors: Nelson, Erica J (Author), Tacchella, Sandro (Author), Diemer, Benedikt (Author), Leja, Joel (Author), Hernquist, Lars (Author), Whitaker, Katherine E (Author), Weinberger, Rainer (Author), Pillepich, Annalisa (Author), Nelson, Dylan (Author), Terrazas, Bryan A (Author), Nevin, Rebecca (Author), Brammer, Gabriel B (Author), Burkhart, Blakesley (Author), Cochrane, Rachel K (Author), van Dokkum, Pieter (Author), Johnson, Benjamin D (Author), Marinacci, Federico (Author), Mowla, Lamiya (Author), Pakmor, Rüdiger (Author), Skelton, Rosalind E (Author), Speagle, Joshua (Author), Springel, Volker (Author), Torrey, Paul (Author), Vogelsberger, Mark (Author), Wuyts, Stijn (Author)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2022-05-06T15:26:49Z.
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