UBC 1610
0.45
UTI
0.44
CN
0.88
Cdens
0.25
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
4.4 [N/pc2]
- CN 0.44 Poorly populated
- Cdens 0.88 Dense
- CC3 0.25 Low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1610 is a poorly populated, dense object of low 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, but with a large variance across recent sources for the metallicity parameter (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 | 91.388 | 28.713 | 0.386 | 1.25 | -3.244 | 23.224 |
| Hu & Soubiran | 2025 | 91.382 | 28.699 | â | â | â | â |
| Zhang et al. | 2024 | 91.394 | 28.703 | â | â | â | â |
| Hunt & Reffert | 2024 | 91.394 | 28.703 | 0.385 | 1.249 | -3.233 | 23.228 |
| Cavallo et al. | 2024 | 91.382 | 28.699 | 0.383 | â | â | â |
| Hunt & Reffert | 2023 | 91.394 | 28.703 | 0.385 | 1.249 | -3.233 | 23.228 |
| Castro-Ginard et al. | 2022 | 91.38 | 28.69 | 0.39 | 1.23 | -3.21 | 26.3 |
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 | 2.54 | 0.35 | 1.41 | 646 | -0.220 | 272 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.220(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.275(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 272(1) | â | â |
| Cavallo et al. | 2024 | 2.54 | 0.35 | â | 646 | 0.500 | â | â | â |
| Hunt & Reffert | 2023 | 2.37 | 0.29 | 1.41 | 757 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 2.89 | 0.36 | â | 231 | 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.