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Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations
Erica J Nelson, Sandro Tacchella, Benedikt Diemer, Joel Leja, Lars Hernquist, Katherine E Whitaker, Rainer Weinberger, Annalisa Pillepich, Dylan Nelson, Bryan A Terrazas, Rebecca Nevin, Gabriel B Brammer, Blakesley Burkhart, Rachel K Cochrane, Pieter Van Dokkum, Benjamin D Johnson, Federico Marinacci, Lamiya Mowla, Rüdiger Pakmor, Rosalind E Skelton
- Center for Astrophysics | Harvard-Smithsonian, Cambridge, MA 02138, USA
- University of Maryland
- Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA
- Cosmic Dawn Center (DAWN), Copenhagen, Denmark
- Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
- Universität Heidelberg
- Niels Bohr Institute, University of Copenhagen, Jagtvej 128, København N, DK-2200, Denmark
- Center for Computational Astrophysics, Flatiron Institute,
- Yale University
- Università di Bologna
- University of Toronto
- Max-Planck-Institut für Astrophysik, 85740 Garching bei München, Germany
- University of Florida
- Massachusetts Institute of Technology
- University of Massachusetts
- University of Colorado
- Pennsylvania State University
- Institute for Computational & Data Sciences, The Pennsylvania State University, University Park, PA, USA
- Rutgers, The State University of New Jersey
Research output: Contribution to journal › Article › peer-review
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