UBC 239
0.66
UTI
0.74
CN
1.0
Cdens
0.75
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
6.5 [N/pc2]
- CN 0.74 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 239 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 123.753 | -30.16 | 0.476 | -3.617 | 1.946 | 34.429 |
| Li et al. | 2025 | 123.763 | -30.155 | 0.467 | -3.623 | 1.947 | â |
| Hu & Soubiran | 2025 | 123.757 | -30.158 | â | â | â | â |
| Hunt & Reffert | 2024 | 123.76 | -30.165 | 0.477 | -3.605 | 1.953 | 41.947 |
| Cavallo et al. | 2024 | 123.756 | -30.158 | 0.477 | â | â | â |
| Hunt & Reffert | 2023 | 123.76 | -30.165 | 0.477 | -3.605 | 1.953 | 41.947 |
| Cantat-Gaudin et al. | 2020 | 123.763 | -30.155 | 0.467 | -3.623 | 1.947 | â |
| Castro-Ginard et al. | 2020 | 123.76 | -30.147 | 0.472 | -3.63 | 1.95 | 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 | 1.84 | 0.285 | 0.39 | 563 | -0.232 | 380 | â | â |
| Li et al. | 2025 | 1.79 | 0.40 | â | 495 | -0.232 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.140(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 380(1) | â | â |
| Cavallo et al. | 2024 | 1.78 | 0.38 | â | 631 | -0.300 | â | â | â |
| Hunt & Reffert | 2023 | 1.89 | 0.13 | 0.39 | 706 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.15 | 0.19 | â | 275 | 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.