Fig. 7
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Rotation curves of the merger remnants for models M1ρ0.25 (p10; panel a) and M4ρ4 (p5; panel b) at different evolutionary times, as indicated. The inset shows, in logarithmic scales, a representative rotation curve of an isolated rotating cluster taken from Kim et al. (2004), illustrating the rapid decline of the rotational velocity beyond Rh.
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