Toward Resolution Convergence for Star Formation and Galactic Winds in Galaxy Simulations

arXiv:2609.34336 · astro-ph.GA, astro-ph.SR · Submitted 2026-09-28 · Read on arXiv

astro-ph.GA, astro-ph.SR

Submitted: 2026-09-28

Updated: 2026-09-28

Terminology

• Core — 13× in this paper · explained in 2 episodes
• Stellar Feedback — 13× in this paper · explained in 2 episodes
• Metallicity — 3× in this paper · explained in 3 episodes
• AGN — 2× in this paper · explained in 1 episode
• Calibration — 2× in this paper · explained in 7 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Giant Molecular Cloud — 2× in this paper
• Hybrid Model — 2× in this paper · explained in 2 episodes
• Hybrid Models — 2× in this paper · explained in 2 episodes
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Aperture — 1× in this paper · explained in 1 episode
• Benchmark — 1× in this paper · explained in 2 episodes
• Benchmarking — 1× in this paper · explained in 4 episodes
• Clustering — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes
• Static Mesh Refinement — 1× in this paper

Sources

• Stellar- and AGN-Driven Outflows in JWST Galaxies at z=3-9: More Frequent, Wider Opening Angles, and Mostly Bounded

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