Table 4: Global parameters of globular clusters of our sample.
Cluster $D_{\rm GC}^{1a}$ MVa HBR2a [Fe/H]a c3a e4a $r_{\rm core}^{5a}$ $r_{\rm tidal}^{6a}$ $\mu_{0,V}^{7a}$ $\sigma^{8b}$ (M/L)b Agec,d Classf
  (kpc) (mag)   (dex)     (pc) (pc) (mag/ $\hbox{$^{\prime\prime}$ }^2$) (km s-1)     (Gyr)
NGC 288 12.0 -6.74 0.98 -1.24 0.96 0.09e 3.64 33.12 19.95 2.9 3.0 11.3 OH
NGC 362 9.4 -8.41 -0.87 -1.16 1.94 0.01 0.47 39.83 14.88 6.4 1.1 8.7 YH
NGC 5286 8.4 -8.61 0.80 -1.67 1.46 0.12 0.93 26.75 16.07 8.0 2.1 NA OH
M 22 4.9 -8.50 0.91 -1.64 1.31 0.14 1.32 26.97 17.32 9.0 3.3 12.3 OH
Terzan 7 16.0 -5.05 -1.00 -0.58 1.08 NA 4.12 49.06 20.65 NA NA 7.4 SG
M 55 3.9 -7.55 0.87 -1.81 0.76 0.02 4.36 25.10 19.13 4.9 3.4 12.3 OH
M 15 10.4 -9.17 0.67 -2.26 2.50 0.05 0.21 64.42 14.21 12.0 2.2 12.3 YH
Palomar 12 15.9 -4.48 -1.00 -0.94 1.94 NA 1.11 96.78 20.59 NA NA 6.4 SG
47 Tuc 7.4 -9.42 -0.99 -0.76 2.03 0.09 0.52 56.1 14.43 11.5 2.0 10.7 BD
M 71 6.7 -5.60 -1.00 -0.73 1.15 0.00 0.73 10.43 19.22 2.3 1.1 10.2 BD
NGC 1904 18.8 -7.86 0.89 -1.57 1.72 0.01 0.60 31.3 16.23 5.4 2.2 11.7 OH
NGC 2808 11.1 -9.39 -0.49 -1.15 1.77 0.12 0.73 43.42 15.17 13.4 2.4 9.3 OH
NGC 3201 8.9 -7.46 0.08 -1.58 1.30 0.12 2.08 41.38 18.77 5.2 4.1 11.3 YH
NGC 5272 12.2 -8.93 0.08 -1.57 1.84 0.04 1.66 115.5 16.34 5.6 1.2 11.3 YH
NGC 5904 6.2 -8.81 0.31 -1.27 1.83 0.14 0.92 61.96 16.05 5.7 1.4 10.9 OH
NGC 6121 5.9 -7.20 -0.06 -1.20 1.59 0.00 0.53 20.79 17.88 4.2 2.6 11.7 OH
NGC 6171 3.3 -7.13 -0.73 -1.04 1.51 0.02 1.01 32.47 18.84 4.1 3.9 11.7 OH
NGC 6205 8.7 -8.70 0.97 -1.54 1.51 0.11 1.75 56.4 16.80 7.1 2.2 11.9 OH
NGC 6254 4.6 -7.48 0.98 -1.52 1.40 0.00 1.10 27.49 17.69 6.6 3.5 11.8 OH
NGC 6637 1.9 -7.64 -1.00 -0.70 1.39 0.01 0.90 22.10 16.83 NA NA 10.6 BD
NGC 6752 5.2 -7.73 1.00 -1.56 2.50 0.04 0.20 64.39 15.20 4.5 1.1 12.2 OH
NGC 6934 12.8 -7.46 0.25 -1.54 1.53 0.01 1.14 38.23 17.26 5.1 2.5 9.6 YH
NGC 7089 10.4 -9.02 0.96 -1.62 1.80 0.11 1.14 71.75 15.92 8.2 1.9 NA OH
NGC 7006 38.8 -7.68 -0.28 -1.63 1.42 0.01 2.90 76.54 18.50 NA NA NA YH
1 Distance from Galactic center; 2 horizontal branch ratio: HBR=(B-R)/(B+V+R); 3 concentration; 4 ellipticity e=1-(b/a); 5 core radius; 6 tidal radius; 7 central surface brightness; 8 central velocity dispersion; a Harris (1996); b Pryor & Meylan (1993); c Rosenberg et al. (1999); d Buonanno et al. (1998); e Frenk & Fall (1982); f Mackey & van den Bergh (2005).


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