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

ABSTRACT 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 (SF...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2021-11, Vol.508 (1), p.219-235
Hauptverfasser:	Nelson, Erica J, Tacchella, Sandro, Diemer, Benedikt, Leja, Joel, Hernquist, Lars, Whitaker, Katherine E, Weinberger, Rainer, Pillepich, Annalisa, Nelson, Dylan, Terrazas, Bryan A, Nevin, Rebecca, Brammer, Gabriel B, Burkhart, Blakesley, Cochrane, Rachel K, van Dokkum, Pieter, Johnson, Benjamin D, Marinacci, Federico, Mowla, Lamiya, Pakmor, Rüdiger, Skelton, Rosalind E, Speagle, Joshua, Springel, Volker, Torrey, Paul, Vogelsberger, Mark, Wuyts, Stijn
Format:	Artikel
Sprache:	eng
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