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Non-ideal magnetohydrodynamic simulations of the first star formation: the effect of ambipolar diffusion

, , , , and . (2022)cite arxiv:2212.08075Comment: 15 pages, 11 figures, 2 tables. Accepted for publication in MNRAS.

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Star formation in turbulent molecular clouds with colliding flow, , and . (Dec 18, 2014)Distortion of Magnetic Fields in Barnard 335, , , , , , , , , and 2 other author(s). (2020)cite arxiv:2001.08542Comment: Accepted for publication in ApJ. arXiv admin note: substantial text overlap with arXiv:1910.09121, arXiv:1912.10029.Improving shock irregularities based on the characteristics of the MHD equations., , and . J. Comput. Phys., 227 (16): 7952-7976 (2008)Non-ideal magnetohydrodynamic simulations of the first star formation: the effect of ambipolar diffusion, , , , and . (2022)cite arxiv:2212.08075Comment: 15 pages, 11 figures, 2 tables. Accepted for publication in MNRAS.Self-gravitational collapse of a magnetized cloud core: high resolution simulations with three-dimensional MHD nested grid., , , and . Comput. Phys. Commun., 164 (1-3): 229-236 (2004)