Table 1
Selected sample of globular clusters.
Globular cluster | d ⊙ | log Tc | log TM | N p | N k | |
|
||||||
NGC 362 | 8.6 | 7.76 | 8.93 | 239 | 8 | |
NGC 7078 (M15) | 10.4 | 7.84 | 9.32 | 310 | 35 | |
NGC 104 (47 Tuc) | 4.5 | 7.84 | 9.55 | 231 | 16 | |
NGC 6121 (M4) | 2.2 | 7.90 | 8.93 | 228 | 10 | |
NGC 6341 (M92) | 8.3 | 7.96 | 9.02 | 118 | 8 | |
|
||||||
NGC 6218 (M12) | 4.8 | 8.19 | 8.87 | 143 | 11 | |
NGC 6254 (M10) | 4.4 | 8.21 | 8.90 | 162 | 6 | |
NGC 6656 (M22) | 3.2 | 8.53 | 9.23 | 143 | 7 | |
NGC 3201 | 4.9 | 8.61 | 9.27 | 80 | 16 | |
NGC 6809 (M55) | 5.4 | 8.90 | 9.29 | 114 | 13 | |
NGC 288 | 8.9 | 8.99 | 9.32 | 85 | 6 | |
|
||||||
NGC 5139 (ω Cen) | 5.2 | 9.60 | 10.09 | 72 | 37 | |
NGC 2419 | 82.6 | 9.87 | 10.63 | 137 | 6 |
Notes. For each globular cluster the following quantities are recorded: distance from the Sun (kpc); logarithm of the core relaxation time (years); logarithm of the half-mass relaxation time (years); number of points in the surface brightness profile; and number of points in the velocity dispersion profile (adapted from ZBV12).
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