Fig. 4.
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Evolution of the distance of the GC from the stellar barycenter of the galaxy for the MOND models without star formation. Each panel corresponds to the galaxy model and each curve to a specific orbit of the GC. The dotted parts of the lines indicate unreliable parts: either the galaxy develops a bar that affects the motion of the GC, or (for GUDG2e7) the GC moves less than three resolution elements from the center.
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