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Table 2
Derived fundamental parameters for the star clusters towards NGC 6357.
| Cluster | AV | Age | d⊙ | RGC | |||||
| (mag) | (Myr) | (kpc) | (kpc) | ||||||
| (1) | (2) | (3) | (4) | (5) | |||||
|
|
|||||||||
| Pismis 24 | 5.87 ± 0.06 | 5 ± 2 | 2.0 ± 0.1 | 5.3 ± 0.1 | |||||
| BDS 101 | 6.57 ± 0.06 | 5 ± 2 | 1.7 ± 0.1 | 5.6 ± 0.1 | |||||
| ESO 392-SC 11 | 6.69 ± 0.06 | 5 ± 2 | 1.9 ± 0.1 | 5.4 ± 0.1 | |||||
| VVV CL164 | 15.9 ± 0.09 | (5 ± 2) × 103 | 1.4 ± 0.1 | 5.9 ± 0.1 | |||||
| VVV CL167 | 4.94 ± 0.06 | 9 ± 2 | 1.6 ± 0.1 | 5.6 ± 0.1 | |||||
Notes. Column 2: AV absorption in the cluster central region. Column 3: age, from VVV photometry. Column 4: distance to the Sun. Column 5: RGC distance of the object to the Galactic center.
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