Global m=1 slow mode in near-Keplerian self-gravitating torus: applications to stellar nuclear disks and AGN molecular tori

arXiv:2604.11528 · astro-ph.GA · Submitted 2026-04-13 · Read on arXiv

astro-ph.GA

Submitted: 2026-04-13

Updated: 2026-10-12

Terminology

• AGN — 2× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• N-body simulations — 1× in this paper · explained in 2 episodes

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