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Modeling the Atomic-to-Molecular Transition and Chemical Distributions of Turbulent Star-Forming Clouds

, , , and . (2013)cite arxiv:1304.7007Comment: 18 pages, 18 Figures, accepted to ApJ.

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Alignment Between Protostellar Outflows and Filamentary Structure, , , , , , , , , and 6 other author(s). (Jul 25, 2017)A multigroup diffusion solver using pseudo transient continuation for a radiation-hydrodynamic code with patch-based AMR., and . J. Comput. Phys., 227 (3): 2154-2186 (2008)The Turbulent Origin of Outflow and Spin Misalignment in Multiple Star Systems, , , , and . (Jun 27, 2016)Modeling the Atomic-to-Molecular Transition and Chemical Distributions of Turbulent Star-Forming Clouds, , , and . (2013)cite arxiv:1304.7007Comment: 18 pages, 18 Figures, accepted to ApJ.The Origin and Universality of the Stellar Initial Mass Function, , , , , , , and . (2013)cite arxiv:1312.5326Comment: 24 pages, 6 figures. Accepted for publication as a chapter in Protostars and Planets VI, University of Arizona Press (2014), eds. H. Beuther, R. S. Klessen, C. P. Dullemond, Th. Henning.Predicting the Radiation Field of Molecular Clouds using Denoising Diffusion Probabilistic Models., , , , , and . CoRR, (2023)ORION2: A magnetohydrodynamics code for star formation., , , , , , , , , and . J. Open Source Softw., 6 (68): 3771 (2021)