Table 5
Galactocentric distances of clusters.
| Cluster | l | b | d⊙ | Ref. | Rgc |
| deg | deg | kpc | kpc | ||
|
|
|||||
| Collinder 261 | 301.684 | −05.528 | 2.75 | 1 | 7.0 |
| IC 4651 | 340.088 | −07.907 | 0.9 | 2 | 7.2 |
| Melotte 66 | 259.559 | −14.244 | 4.5 | 2 | 10.0 |
| NGC 2506 | 230.564 | 09.935 | 3.3 | 1 | 10.4 |
| NGC 2324 | 213.447 | 03.297 | 3.8 | 3 | 11.5 |
| NGC 2477 | 253.563 | −05.838 | 1.5 | 2 | 8.6 |
| NGC 3960 | 294.367 | 06.183 | 2.1 | 4 | 7.4 |
| NGC 4609 | 301.895 | −00.142 | 1.3 | 2 | 7.5 |
| NGC 4815 | 303.625 | −02.097 | 2.5 | 5 | 6.9 |
| NGC 5316 | 310.229 | 00.115 | 1.2 | 2 | 7.4 |
| NGC 6134 | 334.917 | −00.198 | 1.0 | 6 | 7.1 |
| NGC 6253 | 335.460 | −06.251 | 1.6 | 1 | 6.6 |
| NGC 6705 | 27.307 | −02.776 | 1.9 | 7 | 6.3 |
Notes. Distances from the Sun were taken from (1) Bragaglia & Tosi (2006); (2) Kharchenko et al. (2013); (3) Piatti et al. (2004); (4) Bragaglia et al. (2006); (5) Friel et al. (2014); (6) Ahumada et al. (2013); (7) Cantat-Gaudin et al. (2014). The Rgc values were computed with Rgc ⊙ = 8.0 kpc.
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