Fig. 1
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Sketch of the astrophysical setup. A stellar binary (D9) with circumbinary disk is orbiting a SMBH (Sgr A*). Masses (M), eccentricities (e), and semimajor axes (a) are indicated for the inner binary orbit and the outer orbit around the SMBH. The mutual inclination between these orbits is imut and the argument of periapsis of the inner orbit is ωin.
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