OC 0011
0.60
UTI
0.88
CN
1.0
Cdens
1.0
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
451
Core radius and density
1.0 [pc], 36 [pc-2]
- CN 0.88 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
OC 0011 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a very small 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 | 272.992 | -22.964 | 0.614 | 0.46 | 0.81 | 12.11 |
| Hunt & Reffert | 2024 | 272.993 | -22.971 | 0.615 | 0.473 | 0.794 | 11.477 |
| Cavallo et al. | 2024 | 272.982 | -22.963 | 0.615 | â | â | â |
| Hunt & Reffert | 2023 | 272.993 | -22.971 | 0.615 | 0.473 | 0.794 | 11.477 |
| Hao et al. | 2022 | 272.989 | -22.971 | 0.611 | 0.452 | 0.806 | 11.413 |
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 | 1.54 | 3.63 | 3.03 | 1323 | 0.044 | 8978 | â | â |
| Hunt & Reffert | 2024 | 1.54 | 3.33 | 3.03 | 1388 | â | 8978(1) | â | â |
| Cavallo et al. | 2024 | 1.66 | 3.93 | â | 832 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 1.54 | 3.33 | 3.03 | 1387 | â | â | â | â |
| Hao et al. | 2022 | â | 4.79 | â | 1259 | 0.119 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Bronze sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.12 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.12 (50th percentile).