OC 0606
0.40
UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
10.2 [N/pc2]
- CN 0.0 Sparse
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
OC 0606 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is poorly 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 | 212.866 | -63.149 | 0.519 | -5.148 | -2.882 | â |
| Hunt & Reffert | 2024 | 212.897 | -63.141 | 0.508 | -5.141 | -2.888 | â |
| Cavallo et al. | 2024 | 212.906 | -63.139 | 0.507 | â | â | â |
| Hunt & Reffert | 2023 | 212.897 | -63.141 | 0.508 | -5.141 | -2.888 | â |
| Hao et al. | 2022 | 212.897 | -63.146 | 0.535 | -5.181 | -2.83 | 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 | 2.08 | 1.06 | 0.64 | 98 | -0.074 | 227 | â | â |
| Liu et al. | 2025 | 3.08 | 0.47 | â | 76 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 227(1) | â | â |
| Cavallo et al. | 2024 | 2.08 | 0.73 | â | 617 | -0.200 | â | â | â |
| Hunt & Reffert | 2023 | 1.79 | 1.39 | 0.64 | 118 | â | â | â | â |
| Hao et al. | 2022 | â | 1.94 | â | 79 | 0.051 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 312 along with Theia_339.
Palma et al. (2025)
Classified as optical pair (not dynamically associated) P243, along with Theia_339.
Cavallo et al. (2024)
Silver sample.