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B-fields do not suppress star formation in low metallicity dwarf galaxies

, , , , , , , and . (2022)cite arxiv:2210.04922Comment: 19 pages, 19 figures, comments welcome.

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Vertical structure of a supernova-driven turbulent magnetized ISM, , , , , , and . (2012)cite arxiv:1202.0552Comment: Accepted for publication in ApJ.Formation of Molecular Clouds and Global Conditions for Star Formation, , , , , , , , and . (2013)cite arxiv:1312.3223Comment: 25 pages, 7 figures, Accepted for publication as a chapter in Protostars and Planets VI, University of Arizona Press (2014), eds. H. Beuther, R. Klessen, C. Dullemond, Th. Henning.B-fields do not suppress star formation in low metallicity dwarf galaxies, , , , , , , and . (2022)cite arxiv:2210.04922Comment: 19 pages, 19 figures, comments welcome.Gas Loss by Ram Pressure Stripping and Internal Feedback From Low Mass Milky Way Satellites, , , and . (2016)cite arxiv:1605.02746Comment: 16 pages, 7 figures. Accepted for publication in ApJ.Launching Cosmic ray-driven Outflows from the magnetized interstellar medium, , , , , , , , , and 3 other author(s). (2015)cite arxiv:1509.07247Comment: 7 pages, 5 figures, submitted, comments welcome.