Fig. 10.

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Averaged orbit circularity distribution of the ten best-fit models along the long (top) and short (bottom) galaxy axis. The colour indicates the weight of the orbits in phase-space. The dashed lines separate the distribution into cold (λz > 0.8), warm (0.25 < λz < 0.8), hot (|λz|< 0.25), and counter-rotating orbits (λz < −0.25). The red vertical line indicates the effective radius of the NSC.
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