Evolution of superthin galaxies under Milgromian dynamics

arXiv:2608.01632 · astro-ph.GA · Submitted 2026-08-03 · Read on arXiv

astro-ph.GA

Submitted: 2026-08-03

Updated: 2026-09-16

Comments: 15 pages, 12 figures, and 2 tables

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• N-body simulations — 5× in this paper · explained in 2 episodes
• Velocity Dispersion — 5× in this paper · explained in 2 episodes
• Phantom of RAMSES — 3× in this paper
• Core — 2× in this paper · explained in 2 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Benchmark — 1× in this paper · explained in 2 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Disk Initial Conditions Environment — 1× in this paper
• Milky Way — 1× in this paper

Sources

• Modified Newtonian Dynamics: Observational Successes and Failures
• Disc heating: possible link between weak bars and superthin galaxies

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