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Table 1
Basic properties of the GC sample.
| Cluster | [Fe/H]H96 | RVH96 | log (M/M⊙) | [Fe/H]GES | RVGES | N ⋆ |
| (dex) | (km s-1) | (dex) | (dex) | (km s-1) | ||
|
|
||||||
| NGC 104 (47 Tuc) | –0.72 | –18.0 | 6.05±0.04a | –0.71±0.02 | –17.6±0.8 | 119 |
| NGC 362 | –1.36 | 223.5 | 5.53±0.04a | –1.12±0.03 | 222.3±0.6 | 73 |
| NGC 1851 | –1.18 | 320.5 | 5.49±0.04a | –1.07±0.04 | 320.2±0.5 | 89 |
| NGC 1904 (M 79) | –1.60 | 205.8 | 5.20±0.04a | –1.51±0.03 | 205.2±0.5 | 30 |
| NGC 2808 | –1.14 | 101.6 | 5.93±0.05a | –1.03±0.03 | 103.7±1.4 | 45 |
| NGC 4833 | –1.85 | 200.2 | 5.20±0.21b | –1.92±0.03 | 200.6±1.0 | 28 |
| NGC 5927 | –0.49 | –107.5 | 5.32±0.21b | –0.39±0.04 | –102.5±0.7 | 85 |
| NGC 6752 | –1.54 | –26.7 | 5.16±0.21b | –1.48±0.04 | –26.3±0.7 | 57 |
| NGC 7089 (M 2) | –1.65 | –5.3 | 5.84±0.05a | –1.47±0.03 | –1.8±1.3 | 46 |
Notes. The table lists: [Fe/H] and RV from Harris (1996, 2010); the present-day mass from McLaughlin & van der Marel (2005, annotated with a or from Mandushev et al. (1991, annotated with b; the median [Fe/H] and RV from GES data; and the number of GES member stars analyzed.
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