The WEFT project: I. The emergence of turbulence in a cosmic filament

arXiv:2609.17205 · astro-ph.CO · Submitted 2026-09-15 · Read on arXiv

astro-ph.CO

Submitted: 2026-09-15

Updated: 2026-09-15

Comments: Submitted to A&A, 14 pages, 7 figures

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

Terminology

• Accretion Shock — 15× in this paper · explained in 1 episode
• Trace — 8× in this paper · explained in 2 episodes
• Velocity Dispersion — 3× in this paper · explained in 2 episodes
• Accretion Flows — 2× in this paper · explained in 1 episode
• Core — 2× in this paper · explained in 2 episodes
• Abundance — 1× in this paper · explained in 1 episode
• Anisotropy — 1× in this paper · explained in 3 episodes
• Higher-order statistics — 1× in this paper · explained in 2 episodes
• Non-Gaussianity — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes
• Square Kilometre Array — 1× in this paper
• Stellar Feedback — 1× in this paper · explained in 2 episodes

Sources

• Line-Intensity Mapping: 2017 Status Report
• Correcting the hydrostatic mass for non-thermal gas motions: a comparison of two approaches

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