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Table 2
The sample and its internal Vr accuracy.
| Cluster | ⟨ ΔVr ⟩ HR10−HR21 | ⟨ ΔVr ⟩ HR10−HR11 | ⟨ ΔVr ⟩ HR10−HR13 | ⟨ ΔVr ⟩ HR10−HR4 | ⟨ ΔVr ⟩ HR10−HR9A |
| (km s-1) | (km s-1) | (km s-1) | (km s-1) | (km s-1) | |
|
|
|||||
| M 15 | –0.83 (σ = 0.27, 78) | –0.36 (σ = 0.30, 12) | –0.10 (σ = 0.24, 26) | ||
| NGC 4372 | –0.99 (σ = 0.32, 100) | –0.19 (σ = 0.24, 42) | |||
| NGC 4833 | –0.69 (σ = 0.37, 77) | 0.29 (σ = 1.61, 8) | –0.02 (σ = 0.66, 8) | ||
| NGC 6752 | –1.00 (σ = 0.33, 108) | –0.58 (σ = 0.34, 148) | –0.20 (σ = 0.22, 105) | 0.118 (σ = 0.190, 23) | |
| NGC 1851 | –0.94 (σ = 0.39, 91) | –0.30 (σ = 0.25, 51) | –0.67 (σ = 0.31, 56) | 0.15 (σ = 0.35, 52) | |
| NGC 2808 | –0.63 (σ = 0.32, 58) | 0.07 (σ = 0.02, 2) | |||
| NGC 5927 | –0.56 (σ = 0.21, 108) | ||||
|
|
|||||
| Cluster | ⟨ ΔVr ⟩ HR10−HR9B | ⟨ ΔVr ⟩ HR10−HR14A | ⟨ ΔVr ⟩ HR10−HR14B | ⟨ ΔVr ⟩ HR10−HR15N | ⟨ ΔVr ⟩ HR10−HR19A |
| (km s-1) | (km s-1) | (km s-1) | (km s-1) | (km s-1) | |
|
|
|||||
| M 15 | –0.25 (σ = 0.95, 12) | ||||
| NGC 4372 | –0.62 (σ = 0.48, 22) | ||||
| NGC 4833 | |||||
| NGC 6752 | –0.29 (σ = 0.15, 51) | –0.54 (σ = 0.23, 54) | –1.39 (σ = 0.37, 25) | ||
| NGC 1851 | –0.232 (σ = 0.005, 2) | ||||
| NGC 2808 | –0.175 (σ = 0.01, 2) | ||||
| NGC 5927 | |||||
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