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, 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
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/1721.1/142390

Internet

https://hdl.handle.net/1721.1/142390

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