Table 2.
Mean radial velocities of globular clusters.
| Cluster | N | νr | Err | νr (lit.) | Err | Δνr |
|---|---|---|---|---|---|---|
| BH 176 | 11 | 0.1 | 0.7 | 0.0 | 15 | 0.1 |
| Djorg 1 | 3 | −358.1 | 0.7 | −362.4 | 3.6 | 4.2 |
| Djorg 2 | 3 | −159.9 | 0.5 | … | … | … |
| NGC 5634 | 10 | −17.9 | 0.4 | −45.1 | 6.6 | 27.2 |
| NGC 5694 | 9 | −131.5 | 0.6 | −140.3 | 0.8 | 8.8 |
| NGC 5946 | 10 | 114.2 | 0.4 | 128.4 | 1.8 | −14.2 |
| NGC 6256 | 10 | −103.4 | 0.5 | −101.4 | 1.9 | −2.0 |
| NGC 6284 | 7 | 20.7 | 0.4 | 27.5 | 1.7 | −6.8 |
| NGC 6316 | 3 | 92.2 | 0.6 | 71.4 | 8.9 | 20.8 |
| NGC 6352 | 12 | −123.7 | 0.3 | −137.0 | 1.1 | 13.3 |
| NGC 6355 | 7 | −210.3 | 0.4 | −176.9 | 7.1 | −33.4 |
| NGC 6366 | 14 | −118.3 | 0.3 | −122.2 | 0.5 | 3.9 |
| NGC 6401 | 7 | −115.4 | 0.3 | −65.0 | 8.6 | −50.4 |
| NGC 6426 | 7 | −220.0 | 1.0 | −162.0 | 23.0 | −58.0 |
| NGC 6453 | 6 | −110.3 | 0.5 | −83.7 | 8.3 | −26.6 |
| NGC 6517 | 9 | −65.1 | 0.2 | −39.6 | 8.0 | −25.5 |
| NGC 6539 | 9 | 31.3 | 0.4 | 31.0 | 1.7 | 0.3 |
| NGC 6749 | 8 | −51.5 | 0.7 | −61.7 | 2.9 | 10.2 |
| NGC 6864 | 11 | −193.4 | 0.2 | −189.33.6 | −4.1 | |
| Pal 10 | 9 | −29.7 | 0.3 | −31.7 | 0.4 | 2.0 |
| Pal 11 | 7 | −60.0 | 0.4 | −68.0 | 10.0 | 8.0 |
| Pal 14 | 5 | 73.4 | 1.1 | 72.3 | 0.2 | 1.1 |
| Pal 6 | 3 | 177.0 | 1.0 | 181.0 | 2.8 | −4.0 |
| Terzan 1 | 9 | 63.0 | 0.5 | 114.0 | 14.0 | −51.0 |
| Terzan 2 | 3 | 144.6 | 0.8 | 109.0 | 15.0 | 35.6 |
| Terzan 8 | 7 | 142.5 | 0.4 | 130.0 | 8.0 | 12.5 |
| Terzan 9 | 6 | 71.4 | 0.4 | 59.0 | 10.0 | 12.4 |
| Ton 2 | 8 | −172.7 | 0.3 | −184.4 | 2.2 | 11.7 |
Notes. Column 2 gives the number of member stars used to determine the mean radial velocity that is listed in Col. 3. Column 4 lists the standard error of the mean. The radial velocities in the literature (Cols. 5 and 6) are from the Harris catalogue, except for BH 176, for which the source is Sharina et al. (2014). The difference Δνr is given in the last column as FORS2−H10.
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