Table 3
Derived physical parameters from the best-fit one-component models.
| NGC | r tr | R c | r M * | M | log ρ0 | (M/L)V | r α | κ | ||||||
|
|
||||||||||||||
| 104 | 2336 | 3641 | 22.6 | 22.09 | 5.60 | 5.22 | 7.18 | 7.77 | 5.01 | 5.09 | 1.34 | 1.63 | 13.98 | 1.20 |
| 288 | 896 | 835 | 79.42 | 77.32 | 7.50 | 7.53 | 0.74 | 0.76 | 2.04 | 2.09 | 1.88 | 2.20 | 23.82 | 1.61 |
| 362 | 897 | 1600 | 9.88 | 10.75 | 2.65 | 2.26 | 1.87 | 1.81 | 4.83 | 4.78 | 1.05 | 1.09 | 5.35 | 1.26 |
| 2419 | 517 | 1163 | 18.58 | 20.20 | 26.17 | 23.89 | 7.84 | 9.50 | 1.87 | 1.90 | 1.72 | 2.17 | 42.85 | 1.38 |
| 3201 | 1533 | 2278 | 71.58 | 74.77 | 5.12 | 5.03 | 1.31 | 1.10 | 3.01 | 2.98 | 1.91 | 1.99 | 11.29 | 1.28 |
| 5139 | 2861 | 3549 | 127.68 | 163.53 | 10.02 | 10.24 | 26.45 | 31.16 | 3.54 | 3.39 | 1.93 | 2.87 | 19.83 | 1.34 |
| 6121 | 3144 | 2555 | 71.31 | 69.49 | 3.69 | 3.72 | 0.65 | 0.66 | 3.66 | 3.68 | 1.10 | 1.20 | 17.52 | 1.10 |
| 6218 | 982 | 1105 | 47.81 | 50.26 | 3.29 | 3.22 | 0.61 | 0.66 | 3.31 | 3.31 | 1.96 | 1.50 | 8.57 | 1.22 |
| 6254 | 1126 | 2191 | 50.02 | 51.16 | 3.31 | 3.18 | 1.53 | 1.72 | 3.74 | 3.80 | 1.61 | 2.09 | 6.32 | 1.33 |
| 6341 | 724 | 900 | 14.18 | 14.42 | 3.12 | 2.96 | 2.86 | 3.39 | 4.63 | 4.71 | 1.83 | 2.15 | 9.51 | 1.18 |
| 6656 | 2057 | 2224 | 80.92 | 80.74 | 4.18 | 4.17 | 2.08 | 2.14 | 3.64 | 3.65 | 1.11 | 1.11 | 13.95 | 1.16 |
| 6809 | 1072 | 1084 | 110.09 | 109.23 | 5.90 | 5.89 | 0.60 | 0.60 | 2.21 | 2.24 | 1.12 | 1.14 | 12.55 | 1.29 |
| 7078 | 560 | 4289 | 7.51 | 5.46 | 2.97 | 2.88 | 3.98 | 3.95 | 5.21 | 5.54 | 1.12 | 1.22 | 5.62 | 1.28 |
Notes. For each cluster listed in the first column, in double-column
form we provide the relevant physical quantities derived from the King models (as
reported in ZBV12left
columns) and from our truncated anisotropic models
(right columns). In
single-column form, as the final items, we provide the anisotropy radius for the
best-fit models and the global anisotropy
parameter κ. The truncation radius rtr and
the core radius are expressed in units of arcsec; the intrinsic half-mass radius and
the anisotropy radius are expressed in pc. The total mass is expressed in units of
105M⊙ and the central
mass density ρ0 in M⊙
pc-3. Finally, the mass-to-light ratio is given in
solar units M⊙/L⊙.
Most values of the half-mass radii for the King models reported in ZBV12 are incorrect; we report the corrected values.
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