UBC 105
0.64
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
13.4 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 105 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity 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 | 280.324 | -5.425 | 0.473 | 0.483 | -1.019 | -4.57 |
| Li et al. | 2025 | 280.319 | -5.427 | 0.467 | 0.459 | -0.997 | â |
| Hunt & Reffert | 2024 | 280.325 | -5.425 | 0.466 | 0.492 | -1.042 | -5.142 |
| Cavallo et al. | 2024 | 280.335 | -5.426 | 0.469 | â | â | â |
| Hunt & Reffert | 2023 | 280.325 | -5.425 | 0.466 | 0.492 | -1.042 | -5.142 |
| Cantat-Gaudin et al. | 2020 | 280.319 | -5.427 | 0.467 | 0.459 | -0.997 | â |
| Castro-Ginard et al. | 2020 | 280.328 | -5.434 | 0.468 | 0.457 | -0.99 | 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 | 1.8 | 2.41 | 1.83 | 72 | -0.267 | 1114 | â | â |
| Li et al. | 2025 | 1.50 | 2.23 | â | 195 | -0.024 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1114(1) | â | â |
| Cavallo et al. | 2024 | 1.68 | 3.25 | â | 30 | -0.510 | â | â | â |
| Hunt & Reffert | 2023 | 1.92 | 2.59 | 1.83 | 61 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.15 | 1.98 | â | 83 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.