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Table 3

Dimensionless parameters and physical scales of the best-fit models.

King models f(ν) models


NGC  Ψ r0 μ0 V Ψ rscale μ0 V
(1) (2) (3) (4) (5) (6) (7) (8) (9)

104 8.58  ±  0.01 23.09  ±  0.23 14.33  ±  0.01 12.27  ±  0.19 8.21  ±  0.02 250.44  ±  1.46 14.29  ±  0.01 14.07  ±  0.22
288 4.82  ±  0.10 91.03  ±  2.86 20.02  ±  0.03 2.85  ±  0.19 3.91  ±  0.24 79.54  ±  5.37 19.88  ±  0.03 3.70  ±  0.25
362 7.80  ±  0.03 10.21  ±  0.11 14.66  ±  0.01 8.31  ±  0.44 6.86  ±  0.05 52.73  ±  1.09 14.70  ±  0.01 9.26  ±  0.50
2419 6.62  ±  0.04 19.70  ±  0.31 19.43  ±  0.03 5.04  ±  0.43 4.24  ±  0.09 29.86  ±  0.83 19.44  ±  0.04 7.28  ±  0.61
3201 6.17  ±  0.11 76.99  ±  3.05 18.35  ±  0.08 4.28  ±  0.19 4.09  ±  0.40 103.48  ±  11.71 18.33  ±  0.08 5.01  ±  0.23
5139 6.27  ±  0.05 136.94  ±  2.33 16.42  ±  0.04 14.83  ±  0.25 4.31  ±  0.07 150.63  ±  3.07 16.35  ±  0.04 23.41  ±  0.40
6121 7.32  ±  0.07 74.56  ±  1.76 17.00  ±  0.11 4.01  ±  0.30 7.39  ±  0.09 464.49  ±  20.40 17.01  ±  0.11 4.21  ±  0.31
6218 6.11  ±  0.07 51.56  ±  1.51 17.65  ±  0.07 3.93  ±  0.30 4.00  ±  0.14 60.69  ±  2.52 17.57  ±  0.07 5.58  ±  0.42
6254 6.26  ±  0.04 53.63  ±  0.60 16.88  ±  0.09 6.21  ±  0.37 2.67  ±  0.13 51.48  ±  1.45 16.84  ±  0.09 9.69  ±  0.59
6341 7.54  ±  0.02 14.72  ±  0.13 15.31  ±  0.01 9.28  ±  0.41 5.99  ±  0.04 50.00  ±  0.80 15.44  ±  0.01 12.77  ±  0.56
6656 6.47  ±  0.11 86.18  ±  2.34 16.41  ±  0.11 6.47  ±  0.38 5.99  ±  0.26 241.58  ±  26.46 16.41  ±  0.11 7.19  ±  0.42
6809 4.44  ±  0.11 129.11  ±  4.06 19.12  ±  0.04 2.92  ±  0.13 3.92  ±  0.19 101.53  ±  5.39 18.99  ±  0.04 3.61  ±  0.17
7078 8.09  ±  0.02 7.72  ±  0.13 14.07  ±  0.03 11.83  ±  0.24 8.17  ±  0.05 65.88  ±  0.94 13.59  ±  0.06 12.79  ±  0.26

Notes. For each cluster, named in Col. (1), for King and f(ν) models, we list: the concentration parameter Ψ, in other papers often indicated as W0 (Cols. (2) and (6)), the scale radius, expressed in arcsec (r0 in Col. (3) and rscale in Col. (7), as defined in Eqs. (A.2) and (A.5); note that they are intrinsic quantities; they are recorded here in arcseconds, for easier comparison with the observations, as shown in Figs. 13), the V band central surface brightness μ0 in mag arcsec-2 (Cols. (4) and (8)), and the central line-of-sight velocity dispersion V in km s-1 (Cols. (5) and (9)). Formal errors on the various parameters are also recorded (see Appendix B.4).

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