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Fig. 5.

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Demonstration of the approximate equality of the break radii of the GCSs and the a0 radii of their host galaxies. First row: the ratio of the break radius and the MOND a0 radius as a function of the break radius. The vertical axis is in the base-2 logarithmic scale, while the horizontal axis in the base-10 logarithmic scale. The horizontal line indicates the ratio of one (the break and a0 radii are equal). Second row: the same as the first row but for the a0 radii calculated for the Newtonian gravity. Columns: from left to right, the rows show the data derived for all GCs and for the red and blue subpopulations of GCs.

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