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Fig. 1

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Central density ρc as a function of core radius rc for clusters with ρc > 2000 L/pc3 (Harris 1996, update of 2010), with lines of constant Γ (blue) and constant γ (red). Letter labels refer to clusters in Table 1, coloured red if Ns > Nb, blue if Nb > Ns, and yellow if Nb ≃ Ns. Clusters with products of secondary interactions include i) and g), and – indicated in black, with numerical labels – 1: NGC 1851, 2: NGC 6342, 3: NGC 6397 and 4: NGC 6544.

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