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Gone With the Wind: Where is the Missing Stellar Wind Energy from Massive Star Clusters?, , , and . (May 6, 2014)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.The Role of Outflows, Radiation Pressure, and Magnetic Fields in Massive Star Formation, and . (2020)cite arxiv:2006.04829Comment: 21 pages, 16 figures, accepted by ApJ.