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Winds in Star Clusters Drive Kolmogorov Turbulence

, , , , and . (2020)cite arxiv:2006.14626Comment: 12 pages, 5 figures, Submitted to ApJL.

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Winds in Star Clusters Drive Kolmogorov Turbulence, , , , and . (2020)cite arxiv:2006.14626Comment: 12 pages, 5 figures, Submitted to ApJL.GAN-based generative modelling for dermatological applications - comparative study., , , , , , and . CoRR, (2022)Hybrid Adaptive Ray-Moment Method (HARM2): A highly parallel method for radiation hydrodynamics on adaptive grids., , , , and . J. Comput. Phys., (2017)Gone With the Wind: Where is the Missing Stellar Wind Energy from Massive Star Clusters?, , , and . (May 6, 2014)unyt: Handle, manipulate, and convert data with units in Python., , , , and . J. Open Source Softw., 3 (28): 809 (2018)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.ORION2: A magnetohydrodynamics code for star formation., , , , , , , , , and . J. Open Source Softw., 6 (68): 3771 (2021)