For a correct star-centered simulation, every indirect term must be paired with the corresponding direct gravitational force, and the force on a migrating planet should use only the non-axisymmetric part of the disk density.
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On inertial forces (indirect terms) in problems with a central body
For a correct star-centered simulation, every indirect term must be paired with the corresponding direct gravitational force, and the force on a migrating planet should use only the non-axisymmetric part of the disk density.