Fig. 8
The same as Fig. 7 but for NGC 1851, NGC 1904, NGC 5904, NGC 6254, NGC 6171, NGC 6397, NGC 6838, and NGC 7078. The kinematics of some of these clusters has been studied with samples larger than ours, still they lack a study of rotation (NGC 6171, NGC 6397, NGC 6838) or an estimate of the rotation amplitude homogeneous with those obtained here.
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