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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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The formation of the extremely primitive star SDSS J102915+172927 relies on dust, , , , , , and . (2012)cite arxiv:1203.4234Comment: 5 pages, 3 figures, accepted as a Letter to MNRAS.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.The first low-mass stars: critical metallicity or dust-to-gas ratio?, , , and . (2011)cite arxiv:1109.2900 Comment: accepted by MNRAS, 12 pages, 8 figures.Protostellar Feedback and Final Mass of the Second-Generation Primordial Stars, , , and . (2012)cite arxiv:1210.3035Comment: 5 pages, 4 figures, to be published in ApJL.Protostellar Feedback Halts the Growth of the First Stars in the Universe, , , and . (2011)cite arxiv:1111.3649Comment: to appear in Science (published in online Science Express), combined with SOM, additional images and movies are available at http://www-tap.scphys.kyoto-u.ac.jp/~hosokawa/firststarstop_e.html.