Turbulent gas-rich discs at high redshift: the origin of early massive stellar bars

arXiv:2609.03275 · astro-ph.GA · Submitted 2026-09-03 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-03

Updated: 2026-09-03

Terminology

• Metallicity — 4× in this paper · explained in 3 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Momentum transfer — 2× in this paper · explained in 2 episodes
• Stellar Feedback — 2× in this paper · explained in 2 episodes
• Australian Research Council — 1× in this paper
• Benchmark — 1× in this paper · explained in 2 episodes
• National Computing Infrastructure — 1× in this paper
• Population Synthesis — 1× in this paper · explained in 2 episodes

Sources

• The exponential growth of infinitesimal perturbations in the long-term evolution of simulated galaxies
• Resolving the dusty star-forming galaxy GN20 at z=4.055 with NOEMA and JWST: A similar distribution of stars, gas and dust despite distinct apparent profiles
• Galactokinetics
• Regular rotation and low turbulence in a diverse sample of z ~ 4.5 galaxies observed with ALMA
• A massive barred spiral galaxy at z = 5.102 discovered by JWST

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