The birth and fate of stellar clumps in super-early galaxies

arXiv:2609.26993 · astro-ph.GA, astro-ph.CO · Submitted 2026-09-22 · Read on arXiv

astro-ph.GA, astro-ph.CO

Submitted: 2026-09-22

Updated: 2026-09-22

Terminology

• Stellar Feedback — 14× in this paper · explained in 2 episodes
• Velocity Dispersion — 5× in this paper · explained in 2 episodes
• Momentum transfer — 4× in this paper · explained in 2 episodes
• Abundance — 3× in this paper · explained in 1 episode
• Milky Way — 3× in this paper
• Consistency — 2× in this paper · explained in 3 episodes
• Disk Initial Conditions Environment — 2× in this paper
• Trace — 2× in this paper · explained in 2 episodes
• Adam — 1× in this paper · explained in 2 episodes
• Adaptive Mesh Refinement — 1× in this paper
• Gravitational Lensing — 1× in this paper · explained in 2 episodes
• Metallicity — 1× in this paper · explained in 3 episodes
• Non-equilibrium Thermochemistry — 1× in this paper · explained in 2 episodes
• Population Synthesis — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes

Sources

• On the clumpy nature of super-early galaxies

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