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Why stellar feedback promotes disc formation in simulated galaxies

, , , , , and . (2014)cite arxiv:1403.6124Comment: submitted; comments are welcome.

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JADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty, , , , , , , , , and 18 other author(s). (2023)cite arxiv:2308.01230Comment: Submitted to A&A, 25 pages, 13 figures, 4 tables; replaced with updated M_BH-Mstar panel in Fig.7.KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1703.07778Comment: 7 pages, 5 figures, submitted to ApJ Letters.Simulating Trends in Artificial Influence Networks., and . J. Artificial Societies and Social Simulation, (2016)Why stellar feedback promotes disc formation in simulated galaxies, , , , , and . (2014)cite arxiv:1403.6124Comment: submitted; comments are welcome.Bulge-forming galaxies with an extended rotating disk at z~2, , , , , , , , , and 17 other author(s). (2016)cite arxiv:1608.05412Comment: 10 pages, 5 figures, 2 tables, submitted to ApJ.The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^3D$, , , , , , , , , and 20 other author(s). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.