UFMG 22
0.69
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
26.9 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
UFMG 22 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 263.197 | -37.613 | 0.388 | -0.355 | -2.65 | 1.464 |
| Almeida et al. | 2025 | 263.199 | -37.644 | â | â | â | â |
| Hunt & Reffert | 2024 | 263.2 | -37.612 | 0.403 | -0.333 | -2.646 | 33.779 |
| Cavallo et al. | 2024 | 263.186 | -37.611 | 0.401 | â | â | â |
| Hunt & Reffert | 2023 | 263.2 | -37.612 | 0.403 | -0.333 | -2.646 | 33.779 |
| Dias et al. | 2021 | 263.199 | -37.644 | 0.364 | -0.397 | -2.605 | â |
| Ferreira et al. | 2020 | 263.19 | -37.635 | 0.358 | -0.412 | -2.61 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.32 | 3.23 | 2.7 | 22 | 0.035 | 1044 | â | â |
| Almeida et al. | 2025 | 2.33 | 3.23 | â | 12 | â | 623 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1464(1) | â | â |
| Cavallo et al. | 2024 | 2.00 | 4.10 | â | 28 | -0.190 | â | â | â |
| Hunt & Reffert | 2023 | 2.32 | 3.66 | 2.70 | 22 | â | â | â | â |
| Dias et al. | 2021 | 2.33 | 3.23 | â | 12 | 0.259 | â | â | â |
| Ferreira et al. | 2020 | 1.51 | 2.85 | â | 1000 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Silver sample.