UBC 235
0.63
UTI
0.76
CN
0.96
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
4.8 [N/pc2]
- CN 0.76 Rich
- Cdens 0.96 Very dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 235 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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 | 117.334 | -29.34 | 0.572 | -4.215 | 2.792 | 33.753 |
| Li et al. | 2025 | 117.326 | -29.349 | 0.557 | -4.254 | 2.774 | â |
| Hunt & Reffert | 2024 | 117.351 | -29.346 | 0.576 | -4.207 | 2.795 | 53.712 |
| Cavallo et al. | 2024 | 117.303 | -29.316 | 0.575 | â | â | â |
| Hunt & Reffert | 2023 | 117.351 | -29.346 | 0.576 | -4.207 | 2.795 | 53.712 |
| Cantat-Gaudin et al. | 2020 | 117.326 | -29.349 | 0.557 | -4.254 | 2.774 | â |
| Castro-Ginard et al. | 2020 | 117.314 | -29.36 | 0.561 | -4.263 | 2.77 | 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 | 1.645 | 0.84 | 2.41 | 206 | 0.055 | 377 | â | â |
| Li et al. | 2025 | 1.55 | 0.66 | â | 266 | -0.040 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 377(1) | â | â |
| Cavallo et al. | 2024 | 1.64 | 1.03 | â | 229 | 0.150 | â | â | â |
| Hunt & Reffert | 2023 | 1.65 | 0.96 | 2.41 | 182 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.70 | 0.72 | â | 110 | 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.