Recovering pattern speeds of simulated face-on barred galaxies via Schwarzschild modelling

arXiv:2607.29406 · astro-ph.GA · Submitted 2026-07-31 · Read on arXiv

astro-ph.GA

Submitted: 2026-07-31

Updated: 2026-07-31

Comments: Resubmitted to MNRAS after a moderate revision

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

Terminology

• Regularization — 24× in this paper · explained in 3 episodes
• Accuracy — 10× in this paper · explained in 1 episode
• Velocity Dispersion — 6× in this paper · explained in 2 episodes
• Degeneracy — 2× in this paper · explained in 3 episodes
• Anisotropy — 1× in this paper · explained in 3 episodes
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Core — 1× in this paper · explained in 2 episodes
• Generalization — 1× in this paper · explained in 13 episodes
• N-body simulations — 1× in this paper · explained in 2 episodes
• Systematic Bias — 1× in this paper · explained in 3 episodes
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Boxy/peanut/X bulges, barlenses and the thick part of galactic bars: What are they and how did they form?
• Turbulent gas-rich disks at high redshift: bars & bulges in a radial shear flow
• Supermassive black holes in six triaxial galaxies: Insights from SINFONI and MUSE observations

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