A Momentum-Regulated Model For Star Formation Efficiency in Giant Molecular Clouds

arXiv:2607.06727 · astro-ph.SR, astro-ph.GA · Submitted 2026-07-07 · Read on arXiv

astro-ph.SR, astro-ph.GA

Submitted: 2026-07-07

Updated: 2026-07-07

Comments: Accepted for publication in Astronomy & Astrophysics (16 pages, 5 figures)

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

Terminology

Velocity Dispersion — 47× in this paper · explained in 2 episodes
Stellar Feedback — 33× in this paper · explained in 2 episodes
Robustness — 10× in this paper · explained in 5 episodes
Calibration — 5× in this paper · explained in 7 episodes
Clustering — 4× in this paper · explained in 2 episodes
Consistency — 4× in this paper · explained in 3 episodes
Metallicity — 4× in this paper · explained in 3 episodes
Initial Mass Function (IMF) — 1× in this paper · explained in 2 episodes
Lyapunov function — 1× in this paper · explained in 2 episodes
Trace — 1× in this paper · explained in 2 episodes
Unified Framework — 1× in this paper · explained in 5 episodes

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