UBC 122
0.69
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
13.7 [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
UBC 122 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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 | 288.144 | 15.723 | 0.381 | -0.561 | -3.171 | 14.067 |
| Li et al. | 2025 | 288.142 | 15.717 | 0.358 | -0.555 | -3.132 | â |
| Hunt & Reffert | 2024 | 288.138 | 15.731 | 0.381 | -0.577 | -3.183 | 12.373 |
| Cavallo et al. | 2024 | 288.156 | 15.734 | 0.385 | â | â | â |
| Hunt & Reffert | 2023 | 288.138 | 15.731 | 0.381 | -0.577 | -3.183 | 12.373 |
| Cantat-Gaudin et al. | 2020 | 288.142 | 15.717 | 0.358 | -0.555 | -3.132 | â |
| Castro-Ginard et al. | 2020 | 288.144 | 15.71 | 0.352 | -0.568 | -3.135 | 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 | 2.56 | 2.82 | 1.88 | 200 | 0.256 | 1577 | â | â |
| Li et al. | 2025 | 1.94 | 2.74 | â | 310 | -0.039 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1577(1) | â | â |
| Cavallo et al. | 2024 | 2.65 | 2.92 | â | 195 | 0.550 | â | â | â |
| Hunt & Reffert | 2023 | 2.47 | 2.90 | 1.88 | 206 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.67 | 2.40 | â | 51 | 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.