UFMG 65
0.66
UTI
0.57
CN
1.0
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
19.0 [N/pc2]
- CN 0.57 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
UFMG 65 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is poorly studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 258.995 | -33.761 | 0.912 | 1.529 | -1.445 | 1.43 |
| Liu et al. | 2025 | 258.95 | -33.74 | 0.94 | 1.51 | -1.45 | 4.9 |
| Hunt & Reffert | 2024 | 258.952 | -33.743 | 0.937 | 1.509 | -1.446 | 4.904 |
| Cavallo et al. | 2024 | 258.962 | -33.714 | 0.934 | â | â | â |
| Hunt & Reffert | 2023 | 258.952 | -33.743 | 0.937 | 1.509 | -1.446 | 4.904 |
| He et al. | 2022 | 258.525 | -33.498 | 0.924 | 1.613 | -1.667 | â |
| Ferreira et al. | 2021 | 258.947 | -33.75 | 0.899 | 1.538 | -1.455 | 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 | 1.055 | 1.11 | 0.91 | 9 | 0.060 | 117 | â | â |
| Liu et al. | 2025 | 0.95 | 0.35 | â | 21 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 117(1) | â | â |
| Cavallo et al. | 2024 | 1.19 | 1.30 | â | 9 | 0.060 | â | â | â |
| Hunt & Reffert | 2023 | 1.01 | 1.11 | 0.91 | 3 | â | â | â | â |
| He et al. | 2022 | â | 1.10 | â | 6 | â | â | â | â |
| Ferreira et al. | 2021 | 1.10 | 3.56 | â | 200 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 389 along with HSC_2911, and of multiple system 16 along with HSC_2911 and BH_221.
Palma et al. (2025)
Part of multiple system G14, along with CWNU_170, HSC_2911 and BH_221.
Cavallo et al. (2024)
Bronze sample.