Fig. 3

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Value of the Hamiltonian εℬq(r) in Eq. (35) as a function of the parametrisation point, q, and the star’s instantaneous position, r. The value of εℬq(r) is shown by the colour shades and black level curves. By definition of q, the value of εℬq(r) is zero along the diagonal (i.e. for r = q). An example of the periapsis, rp, apoapsis, ra, and best parametrisation point, q⋆, are shown in red and blue. In this system of units, the Plummer characteristic radius, κ, lies at r = 1.
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