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Fig. 7

image

Top: axis ratio of the stellar component of the galaxy remnants versus the averaged tidal radius in units of the averaged half-mass radius. Bottom: ratio of the rotational peak velocity and the mean velocity dispersion of the galaxy remnants versus the averaged tidal radius in units of the averaged half-mass radius of the stellar component. Both panels only contain simulations without any inclination between orbital plane and galactic disk. Open symbols represent simulations without encounters with other cluster members.

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