In isolated MOND simulations, the UGC 7321 model keeps h_z/R_D mostly below 0.1 for 5 Gyr, and higher-MOND-depth (more diffuse) models stay thinner than low-depth models.
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Evolution of superthin galaxies under Milgromian dynamics
In isolated MOND simulations, the UGC 7321 model keeps h_z/R_D mostly below 0.1 for 5 Gyr, and higher-MOND-depth (more diffuse) models stay thinner than low-depth models.