Dynamical constraints on the S2 (S0-2) star possible companions

arXiv:2512.11046 · astro-ph.GA, astro-ph.EP, astro-ph.SR · Submitted 2025-12-11 · Read on arXiv

astro-ph.GA, astro-ph.EP, astro-ph.SR

Submitted: 2025-12-11

Updated: 2025-12-11

Terminology

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

Sources

• Measuring the effects of General Relativity at the Galactic Center with Future Extremely Large Telescopes
• Extensions of Brown Hamiltonian-I. A high-accuracy model for von Zeipel-Lidov-Kozai oscillations

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