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Table 3.
Derived cluster mean properties.
| Cluster | n | RV (*) | [Fe/H]C04 |
|---|---|---|---|
| (km s−1) | (dex) | ||
| K28 | 11 | 132.80 ± 1.61 | −0.94 ± 0.03 |
| K44 | 11 | 143.70 ± 0.83 | −0.78 ± 0.03 |
| L11 | 5 | 126.28 ± 1.66 | −0.83 ± 0.06 |
| L32 | 4 | 120.28 ± 3.37 | −0.96 ± 0.04 |
| L38 | 5 | 152.93 ± 1.50 | −1.39 ± 0.03 |
| L116 | 2 | 153.44 ± 2.55 | −0.89 ± 0.02 |
| N152 | 6 | 148.41 ± 2.43 | −0.72 ± 0.02 |
| NGC 339 | 13 | 103.30 ± 2.35 | −1.15 ± 0.02 |
| NGC 361 | 11 | 161.18 ± 1.24 | −0.90 ± 0.03 |
| NGC 411 | 4 | 140.72 ± 3.89 | −0.74 ± 0.04 |
| NGC 416 | 8 | 138.04 ± 1.25 | −0.85 ± 0.04 |
| NGC 419 | 5 | 171.48 ± 2.53 | −0.62 ± 0.02 |
Notes.
(*)
For the clusters of our sample common to Song et al. (2021) our RV values are systematically smaller, probably due to the correction for off-centering of the stars in the slit.
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