Non-resonant relaxation of rotating globular clusters

Open Access

Fig. A.2.

Illustration of the frames used to compute the argument of the background DF, $F_{rot} (E^{'}, L^{'}, L_{z}^{'})$ $F_{{\rm rot}} (E^\prime, L^\prime , L_{z}^\prime)$ . In the left panel, the cluster is seen from the side of the rotation plane, (Oxy). In the right panel, the (OXY)-plane is the orbital plane of the test star, seen from above.

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