The paper introduces a modified Laplace-Lagrange formula, Eq. (10), that adds the Heppenheimer eccentricity factor to handle eccentric companion stars, and extends it to multiple perturbers via superposition.
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Analytical estimates of secular frequencies for binary star systems
The paper introduces a modified Laplace-Lagrange formula, Eq. (10), that adds the Heppenheimer eccentricity factor to handle eccentric companion stars, and extends it to multiple perturbers via superposition.