OC 0266
0.29
UTI
0.49
CN
0.32
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
49
Core radius and density
2.0 [pc], 1.6 [pc-2]
- CN 0.49 Poorly populated
- Cdens 0.32 Loose
- CC3 0.5 Intermediate quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
OC 0266 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (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 | 51.168 | 54.9 | 0.43 | 0.287 | -1.02 | 19.573 |
| Hunt & Reffert | 2024 | 51.207 | 54.942 | 0.424 | 0.299 | -0.99 | 17.312 |
| Cavallo et al. | 2024 | 51.092 | 54.909 | 0.426 | â | â | â |
| Hunt & Reffert | 2023 | 51.207 | 54.942 | 0.424 | 0.299 | -0.99 | 17.312 |
| Hao et al. | 2022 | 51.117 | 54.893 | 0.443 | 0.331 | -1.035 | -26.659 |
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 | 2.16 | 3.62 | 2.47 | 68 | 0.319 | 1013 | â | â |
| Hunt & Reffert | 2024 | 2.16 | 3.60 | 2.47 | 68 | â | 1013(1) | â | â |
| Cavallo et al. | 2024 | 2.40 | 3.64 | â | 49 | 0.440 | â | â | â |
| Hunt & Reffert | 2023 | 2.16 | 3.60 | 2.47 | 68 | â | â | â | â |
| Hao et al. | 2022 | â | 4.36 | â | 126 | 0.198 | 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 class: 0.22 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.22 (50th percentile).