Effects of resolution and local stability on galactic disks: Halo resolution and softening on bar formation

arXiv:2603.02494 · astro-ph.GA · Submitted 2026-03-03 · Read on arXiv

astro-ph.GA

Submitted: 2026-03-03

Updated: 2026-08-26

Comments: 15 pages, 12 figures. Published in A&A

Journal ref: A&A, 712, A38 (2026)

DOI: 10.1051/0004-6361/202659676

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

Terminology

Velocity Dispersion — 20× in this paper · explained in 2 episodes
Momentum transfer — 12× in this paper · explained in 2 episodes
Stellar Feedback — 4× in this paper · explained in 2 episodes
Angular Momentum Loss — 3× in this paper · explained in 1 episode
Anisotropy — 3× in this paper · explained in 3 episodes
N-body simulations — 3× in this paper · explained in 2 episodes
Angular Momentum Transport — 2× in this paper · explained in 3 episodes
Core — 2× in this paper · explained in 2 episodes
Trace — 2× in this paper · explained in 2 episodes
Accuracy — 1× in this paper · explained in 1 episode
Alignment — 1× in this paper · explained in 1 episode
Clustering — 1× in this paper · explained in 2 episodes
Phase Transitions — 1× in this paper · explained in 2 episodes

Sources

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