Table 1
Selected globular clusters.
Globular cluster | d⊙ | C | log Tc | log TM | e | vrot | Nv | Ne |
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Ref. |
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NGC 362 | 8.6 | 1.76 | 7.76 | 8.93 | 0.01 | 0.0 | 208 | 92 | 4.22 | 0.33 | (1) |
NGC 7078 (M 15) | 10.4 | 2.29 | 7.84 | 9.32 | 0.05 | 1.7 | 1777 | 1298 | 16.94 | 0.62 | (2) |
NGC 104 (47 Tuc) | 4.5 | 2.07 | 7.84 | 9.55 | 0.09 | 2.2 | 2638 | 709 | 19.27 | 1.44 | (3), (4) |
NGC 6121 (M 4) | 2.2 | 1.65 | 7.90 | 8.93 | 0.00 | 0.9 | 200 | 55 | 10.36 | 0.87 | (4) |
NGC 6341 (M 92) | 8.3 | 1.68 | 7.96 | 9.02 | 0.10 | 2.5 | 295 | 42 | 13.96 | 1.14 | (5) |
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NGC 6218 (M 12) | 4.8 | 1.34 | 8.19 | 8.87 | 0.04 | 0.15 | 242 | 58 | 10.38 | 1.06 | (4) |
NGC 6254 (M 10) | 4.4 | 1.38 | 8.21 | 8.90 | 0.00 | ... | 147 | 47 | 5.22 | 0.55 | (6) |
NGC 6656 (M 22) | 3.2 | 1.38 | 8.53 | 9.23 | 0.14 | 1.5 | 345 | 116 | 8.40 | 0.88 | (4) |
NGC 3201 | 4.9 | 1.29 | 8.61 | 9.27 | 0.12 | 1.2 | 399 | 201 | 10.35 | 1.27 | (7) |
NGC 6809 (M 55) | 5.4 | 0.93 | 8.90 | 9.29 | 0.02 | 0.25 | 728 | 311 | 7.79 | 1.44 | (4) |
NGC 288 | 8.9 | 0.99 | 8.99 | 9.32 | ... | 0.25 | 171 | 68 | 5.53 | 0.93 | (4), (6) |
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NGC 5139 (ω Cen) | 5.2 | 1.31 | 9.60 | 10.09 | 0.17 | 7.9 | 2060 | 554 | 5.97 | 0.62 | (8), (9) |
NGC 2419 | 82.6 | 1.37 | 9.87 | 10.63 | 0.03 | 0.6 | 166 | 38 | 14.63 | 1.74 | (10) |
Notes. From left to right, the following quantities are displayed: distance from the Sun (kpc), concentration parameter, logarithm of the core relaxation time (years), logarithm of the half-mass relaxation time (years), ellipticity, rotational velocity (km s-1), total number of velocity data-points available, number of velocity data-points inside the projected half-light radius, ratio of the radius of the outermost velocity point to the projected half-light radius, and ratio of the radius of the outermost velocity point to the truncation radius. The sources of the kinematical data are listed in the last column (see main text for references of the other quantities).
References. (1) Fischer et al. (1993); (2) Gebhardt et al. (2000); (3) Gebhardt et al. (1995); (4) Lane et al. (2011); (5) Drukier et al. (2007); (6) Carretta et al. (2009); (7) Cote et al. (1995); (8) Mayor et al. (1997); (9) Reijns et al. (2006); (10) Ibata et al. (2011).
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