The driving mode of turbulence in disc galaxy simulations with adaptive mesh refinement

arXiv:2609.15041 · astro-ph.GA, astro-ph.IM · Submitted 2026-09-14 · Read on arXiv

astro-ph.GA, astro-ph.IM

Submitted: 2026-09-14

Updated: 2026-09-14

Comments: 11 pages, 11 figures, submitted to MNRAS

Code: https://github.com/James471/TurbulenceScripts

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

Terminology

• Anti-correlation — 7× in this paper · explained in 3 episodes
• Large Magellanic Cloud — 3× in this paper
• Stellar Feedback — 2× in this paper · explained in 2 episodes
• Cooperation — 1× in this paper · explained in 2 episodes
• Large Language Model (LLM) — 1× in this paper · explained in 3 episodes

Sources

• The Star Formation Rate of Molecular Clouds

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