UFMG 41
0.59
UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
29.8 [N/pc2]
- CN 0.5 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
UFMG 41 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (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 | 235.116 | -55.75 | 0.534 | -1.053 | -1.884 | -28.669 |
| Almeida et al. | 2025 | 235.135 | -55.75 | â | â | â | â |
| Hunt & Reffert | 2024 | 235.117 | -55.754 | 0.548 | -1.043 | -1.845 | -28.67 |
| Cavallo et al. | 2024 | 235.128 | -55.758 | 0.546 | â | â | â |
| Hunt & Reffert | 2023 | 235.117 | -55.754 | 0.548 | -1.043 | -1.845 | -28.67 |
| Dias et al. | 2021 | 235.135 | -55.75 | 0.506 | -1.017 | -1.895 | â |
| Ferreira et al. | 2020 | 235.14 | -55.729 | 0.503 | -1.026 | -1.897 | 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 | 1.77 | 3.37 | 1.73 | 74 | 0.087 | 288 | â | â |
| Almeida et al. | 2025 | 1.77 | 3.15 | â | 73 | â | 156 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 421(1) | â | â |
| Cavallo et al. | 2024 | 1.85 | 3.76 | â | 74 | -0.020 | â | â | â |
| Hunt & Reffert | 2023 | 1.72 | 3.37 | 1.73 | 89 | â | â | â | â |
| Dias et al. | 2021 | 1.77 | 3.15 | â | 73 | 0.194 | â | â | â |
| Ferreira et al. | 2020 | 1.45 | 3.91 | â | 158 | 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: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.