The galactic acceleration scale is imprinted on globular cluster systems of early-type galaxies of most masses and on red and blue globular cluster subpopulations

Open Access

Fig. 3.

Statistically significant correlations of the break radii of GCSs with the properties of their host galaxies. From top to bottom: stellar mass, effective radius, Sérsic index, MOND a₀ radius, Newtonian a₀ radius. The open symbols indicate suspicious measurements. The red numbers in the corners indicate the p-value of the Spearman’s correlations.

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