Table 8
Comparison between the values of structural parameters from best-fit King models found in this paper and in previous studies.
| NGC | Ref. | Ψ | r0 | μ0 | V | NGC | Ref. | Ψ | r0 | μ0 | V | |
|
|
|
|||||||||||
| 104 | (0) | 8.58 | 23.09 | 14.33 | 12.27 | 288 | (0) | 4.82 | 91.03 | 20.02 | 2.85 | |
| (1) | 9.33 | 15.25 | 14.42 | 11.5 | (1) | 4.33 | 94.05 | 20.00 | 2.9 | |||
| (2) | 8.70 | 22.84 | 14.42 | ... | (2) | 4.65 | 98.41 | 20.00 | ... | |||
| (3) | 8.6 | 23.19 | 14.36 | 15.27 | (3) | 4.8 | 92.87 | 20.00 | 2.79 | |||
| (4) | 8.81 | 22.01 | 14.38 | 11.0 | (4) | 4.80 | 92.79 | 20.05 | 2.9 | |||
| 362 | (0) | 7.80 | 10.21 | 14.66 | 8.31 | 2419 | (0) | 6.62 | 19.70 | 19.43 | 5.04 | |
| (1) | 8.93 | 7.19 | 14.79 | 6.4 | (1) | 6.55 | 19.88 | 19.77 | 3.0 | |||
| (2) | 6.80 | 10.79 | 14.79 | ... | (2) | 6.55 | 22.19 | 19.77 | ... | |||
| (3) | 7.9 | 10.05 | 14.66 | 11.12 | (3) | 6.5 | 20.60 | 19.44 | 5.32 | |||
| (4) | 7.76 | 11.16 | 14.80 | 6.4 | (4) | 6.44 | 20.47 | 19.67 | 4.0 | |||
| 3201 | (0) | 6.17 | 76.99 | 18.35 | 4.28 | 5139 | (0) | 6.27 | 136.94 | 16.42 | 14.83 | |
| (1) | 6.17 | 86.22 | 18.96 | 5.2 | (1) | 5.77 | 157.85 | 16.81 | 16.0 | |||
| (2) | 6.21 | 93.55 | 18.96 | ... | (2) | 5.94 | 168.01 | 16.81 | ... | |||
| (3) | 6.1 | 77.68 | 18.30 | 4.21 | (3) | 6.2 | 141.20 | 16.44 | 13.75 | |||
| (4) | 6.14 | 83.98 | 19.00 | 5.0 | (4) | 6.21 | 152.73 | 16.81 | 16.8 | |||
| 6121 | (0) | 7.32 | 74.56 | 17.00 | 4.01 | 6218 | (0) | 6.11 | 51.56 | 17.65 | 3.93 | |
| (1) | 7.24 | 45.38 | 17.88 | 4.2 | (1) | 6.55 | 37.57 | 18.00 | 4.5 | |||
| (2) | 7.20 | 52.37 | 17.88 | ... | (2) | 6.48 | 42.38 | 18.00 | ... | |||
| (3) | 7.4 | 72.57 | 16.94 | 5.25 | (3) | 6.1 | 51.74 | 17.62 | 4.66 | |||
| (4) | 7.40 | 72.42 | 17.95 | 4.0 | (4) | 6.33 | 50.70 | 18.10 | 4.5 | |||
| 6254 | (0) | 6.26 | 53.63 | 16.88 | 6.21 | 6341 | (0) | 7.54 | 14.72 | 15.31 | 9.28 | |
| (1) | 6.55 | 48.45 | 17.70 | 6.6 | (1) | 8.22 | 11.27 | 15.46 | 5.9 | |||
| (2) | 6.55 | 54.49 | 17.70 | ... | (2) | 7.92 | 14.56 | 15.46 | ... | |||
| (3) | 6.5 | 49.41 | 16.85 | 6.17 | (3) | 7.5 | 16.15 | 15.61 | 8.71 | |||
| (4) | 6.48 | 49.19 | 17.70 | 6.6 | (4) | 7.50 | 16.20 | 15.47 | 6.0 | |||
| 6656 | (0) | 6.47 | 86.18 | 16.41 | 6.47 | 6809 | (0) | 4.44 | 129.11 | 19.12 | 2.92 | |
| (1) | 6.17 | 83.19 | 17.40 | 9.0 | (1) | 3.17 | 192.94 | 19.40 | 4.9 | |||
| (2) | 6.21 | 91.41 | 17.40 | ... | (2) | 3.53 | 215.54 | 19.40 | ... | |||
| (3) | 6.5 | 85.15 | 16.38 | 8.56 | (3) | 4.5 | 126.41 | 19.07 | 3.73 | |||
| (4) | 6.48 | 84.96 | 17.42 | 7.8 | (4) | 4.49 | 126.22 | 19.36 | 4.0 | |||
| 7078 | (0) | 8.09 | 7.72 | 14.07 | 11.83 | |||||||
| (1) | 12.32 | 1.96 | 14.21 | 12.0 | ||||||||
| (2) | 10.75 | 4.09 | 14.21 | ... | ||||||||
| (4) | 9.72 | 8.49 | 14.21 | 13.5 | ||||||||
Notes. See Table 3 for the description of column entries. For NGC 7078 the entry marked with (3) is missing: the authors of this work decided to exclude this globular cluster from their analysis because it is core-collapsed. In references (2) and (4) only the core radii are given; therefore we used the values of Rc and Ψ to calculate r0 (see Appendix A.1).
References. (0) This work; (1) Pryor & Meylan (1993); (2) Trager et al. (1995); (3) McLaughlin & van der Marel (2005); (4) Harris (2010).
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