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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.

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The Necessity of Feedback Physics in Setting the Peak of the Initial Mass Function, , and . (Oct 16, 2015)Mass Transport and Turbulence in Gravitationally Unstable Disk Galaxies II: The Effects of Star Formation Feedback, , and . (2016)cite arxiv:1605.00646Comment: 16 pages, 13 figures. Resubmitted to the Astrophysical Journal after responding to referee comments. 6 TB of simulation data and processed derived data are available at http://dx.doi.org/10.13012/J85Q4T1T. An interactive data exploration widget is available at https://demo.use.yt (click "galaxy_visualization.ipynb"; once the Jupyter notebook launches, click "Cell -> Run All").Hybrid Adaptive Ray-Moment Method (HARM$^2$): A Highly Parallel Method for Radiation Hydrodynamics on Adaptive Grids, , , , and . (2016)cite arxiv:1607.01802Comment: 27 pages, 8 figures, submitted to Journal of Computational Physics. Referee comments received and will be addressed in final version.Star Formation in Atomic Gas. (2012)cite arxiv:1208.1504Comment: 9 pages, 8 figures, submitted to ApJ.Line Emission from Radiation-Pressurized HII Regions I: Internal Structure and Line Ratios, , , , and . (2013)cite arxiv:1303.4742Comment: 8 pages, 4 figures, accepted for publication in ApJ.The Star Formation Law in Molecule-Poor Galaxies. (2013)cite arxiv:1309.5100Comment: 18 pages, 9 figures, accepted for publication in MNRAS.The Big Problems in Star Formation: the Star Formation Rate, Stellar Clustering, and the Initial Mass Function. (2014)cite arxiv:1402.0867Comment: 88 pages, 19 figures, review article in press for Physics Reports.SLUG - Stochastically Lighting Up Galaxies. II: Quantifying the Effects of Stochasticity on Star Formation Rate Indicators, , and . (2014)cite arxiv:1403.4605Comment: 13 pages, 8 figures. Submitted to MNRAS. Comments are welcome.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.Evolution of Blister-Type HII Regions in a Magnetized Medium, and . (2011)cite arxiv:1110.4645 Comment: 15 pages, 17 figures, 1 table.