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Fig. 18

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Jeans models for the blue GCs (sample BlueFinal, β = 0) for a Burkert dark matter halo. The cross marks the best-fit parameters (cf. Table 9). The thick solid, dashed and thin solid lines indicate the 68, 90 and 99 per cent confidence limits. The thick dot-dashed line indicates the Donato et al. (2009) central dark matter surface density relation log μ0D = 2.15  ±  0.2    [log (M   pc-2)]  (the thin dot-dashed lines show the uncertainties).

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