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Cited article:

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The dynamical state of bars in cluster dwarf galaxies: the cases of NGC 4483 and NGC 4516

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Simulations of star-forming main-sequence galaxies in Milgromian gravity

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Properties of Fast and Slow Bars Classified by Epicyclic Frequency Curves from Photometry of Barred Galaxies

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A slow lopsided bar in the interacting dwarf galaxy IC 3167

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Simulated Bars May Be Shorter but Are Not Slower Than Those Observed: TNG50 versus MaNGA

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Fast galaxy bars continue to challenge standard cosmology

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