OC 0351
0.26
UTI
0.0
CN
0.17
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
9.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.17 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
OC 0351 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below 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.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 96.17 | -1.351 | 0.522 | -0.68 | 1.925 | 30.306 |
| Hu & Soubiran | 2025 | 96.24 | -1.346 | â | â | â | â |
| Hunt & Reffert | 2024 | 96.144 | -1.349 | 0.516 | -0.692 | 1.927 | 27.306 |
| Cavallo et al. | 2024 | 96.239 | -1.346 | 0.516 | â | â | â |
| Hunt & Reffert | 2023 | 96.144 | -1.349 | 0.516 | -0.692 | 1.927 | 27.306 |
| Hao et al. | 2022 | 96.12 | -1.282 | 0.529 | -0.663 | 1.872 | 31.376 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.220* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 100* | â | â |
| Cavallo et al. | 2024 | 1.94 | 0.93 | â | 871 | 0.210 | â | â | â |
| Hunt & Reffert | 2023 | 1.82 | 0.72 | 0.33 | 1081 | â | â | â | â |
| Hao et al. | 2022 | â | 1.25 | â | 794 | 0.611 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.