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Radiation-Hydrodynamic Simulations of the Formation of Massive Star Clusters I. Implications for the Origin of the Initial Mass Function, , and . (2011)cite arxiv:1104.2038 Comment: 15 pages, 11 figures, submitted to ApJ.The Effects of Magnetic Fields and Protostellar Feedback on Low-mass Cluster Formation, , , and . (2017)cite arxiv:1709.01277Comment: submitted to MNRAS.Magnetized Interstellar Molecular Clouds. I. Comparison Between Simulations and Zeeman Observations, , and . (Jun 26, 2015)Bondi-Hoyle Accretion in an Isothermal Magnetized Plasma, , , and . (Jan 27, 2014)Feedback Effects on Low-Mass Star Formation, , , and . (2012)cite arxiv:1201.2751Comment: 20 pages, 20 figures.The Global Evolution of Giant Molecular Clouds II: The Role of Accretion, , , and . (2011)cite arxiv:1105.6097 Comment: 23 Pages, 9 Figures. Resubmitted to ApJ with referee comments. Comments are welcome.Radiation-Hydrodynamic Simulations of the Formation of Orion-Like Star Clusters II. The Initial Mass Function from Winds, Turbulence, and Radiation, , and . (2012)cite arxiv:1203.2620Comment: 17 pages, 15 figures, emulateapj format, submitted to ApJ. For movies of the results, see http://www.ucolick.org/~krumholz/downloads.html.Massive Warm/Hot Galaxy Coronae as Probed by OVI, OVII and OVIII Absorbers, , and . (2016)cite arxiv:1602.00689Comment: 13 pages, 5 figures. Submitted to ApJ, comments welcome.The formation of the first stars and galaxies, , , and . Nature, (2009)What Physics Determines the Peak of the IMF? Insights from the Structure of Cores in Radiation-Magnetohydrodynamic Simulations, , , and . (2016)cite arxiv:1603.04557Comment: 10 pages, 8 figures, submitted to MNRAS.