Fig. 17.

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Comparison of observed and expected stellar velocities, and the stellar velocity dispersion, along the major axis of NGC 4751. The blue line shows the predicted circular velocity extracted from a KinMS model built using of parameters of our adopted result (see text for the details). The black line shows the (deprojected for an inclination of 66°) velocity of the stars, and the red line the velocity dispersion of the stars.
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