OC 0126
0.27
UTI
0.25
CN
0.15
Cdens
0.75
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
25
Core radius and density
2.4 [pc], 0.8 [pc-2]
- CN 0.25 Poorly populated
- Cdens 0.15 Very loose
- CC3 0.75 High quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
OC 0126 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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 rarely studied in the literature.
Note: This object shares a large 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 | 304.459 | 42.115 | 0.584 | -1.669 | -3.156 | -20.874 |
| Hu & Soubiran | 2025 | 304.445 | 42.141 | â | â | â | â |
| Hunt & Reffert | 2024 | 304.466 | 42.147 | 0.585 | -1.683 | -3.147 | -12.578 |
| Cavallo et al. | 2024 | 304.445 | 42.141 | 0.587 | â | â | â |
| Hunt & Reffert | 2023 | 304.466 | 42.147 | 0.585 | -1.683 | -3.147 | -12.578 |
| Hao et al. | 2022 | 304.466 | 42.15 | 0.594 | -1.668 | -3.153 | -25.625 |
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 | 1.64 | 1.79 | 1.33 | 811 | 0.161 | 117 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.220(5) | â | â | â |
| Hunt & Reffert | 2024 | 1.64 | 1.77 | 1.33 | 811 | â | 117(1) | â | â |
| Cavallo et al. | 2024 | 1.58 | 1.81 | â | 1175 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 1.64 | 1.77 | 1.33 | 811 | â | â | â | â |
| Hao et al. | 2022 | â | 5.12 | â | 794 | 0.161 | 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.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.13 (50th percentile), true positive (human-assigned).
Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.13 (50th percentile), true positive (human-assigned).