A power-law thin disk around Sgr A* induces secular Δp, extra in-plane precession, and out-of-plane precession that can compete with Lense-Thirring on S301 and must be constrained with S2.
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Effects of a disk structure on stellar motion at the Galactic Center
A power-law thin disk around Sgr A* induces secular Δp, extra in-plane precession, and out-of-plane precession that can compete with Lense-Thirring on S301 and must be constrained with S2.