Disc-mediated angular momentum transport resolves the mass-gain problem in rotating binaries

arXiv:2609.30230 · astro-ph.SR · Submitted 2026-09-24 · Read on arXiv

astro-ph.SR

Submitted: 2026-09-24

Updated: 2026-09-24

Terminology

• Angular Momentum Transport — 24× in this paper · explained in 3 episodes
• Metallicity — 22× in this paper · explained in 3 episodes
• Core — 8× in this paper · explained in 2 episodes
• Trace — 4× in this paper · explained in 2 episodes
• Momentum transfer — 3× in this paper · explained in 2 episodes
• Ablation — 2× in this paper · explained in 1 episode
• alpha — 2× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Angular Momentum Loss — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Inverse Problem — 1× in this paper · explained in 2 episodes
• Population Synthesis — 1× in this paper · explained in 2 episodes
• Small Magellanic Cloud — 1× in this paper

Sources

• You're Gonna Need a Bigger Core: Calibrating Massive Star Models against Galactic OB-type Stars

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