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Fig. 13.

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Evolutionary scheme we propose for CGs. In the x-axis we have the velocity dispersion of CG, in the opposite direction the crossing time which increases as σG decreases, having less dynamically evolved CGs. On the y-axis, we have the fraction of LTGs. Our scheme evolves from stages 1 to 3, where the CGs have a lower fraction of LTGs, higher σ, and lower Hotc. Our results show that this evolution is accelerated in non-isolated CGs.

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