OC 0467
0.09
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.3
Clit
0.14
Cdup
Stellar density (N50/rad)
69.9 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.3 Poorly studied
- Cdup 0.14 Likely duplicate
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
OC 0467 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption and metallicity parameters (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously 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 | 129.403 | -40.295 | 1.058 | -5.668 | 3.694 | 19.988 |
| Liu et al. | 2025 | 129.41 | -40.29 | 1.05 | -5.66 | 3.68 | 22.22 |
| Hunt & Reffert | 2024 | 129.408 | -40.292 | 1.054 | -5.656 | 3.675 | 22.223 |
| Cavallo et al. | 2024 | 129.4 | -40.289 | 1.058 | â | â | â |
| Hunt & Reffert | 2023 | 129.408 | -40.292 | 1.054 | -5.656 | 3.675 | 22.223 |
| Hao et al. | 2022 | 129.381 | -40.288 | 1.083 | -5.649 | 3.723 | 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 | 0.96 | 1.135 | 2.11 | 4 | 0.079 | 296 | â | â |
| Liu et al. | 2025 | 1.43 | 0.34 | â | 7 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 296(1) | â | â |
| Cavallo et al. | 2024 | 0.96 | 1.20 | â | 2 | -0.380 | â | â | â |
| Hunt & Reffert | 2023 | 0.88 | 1.07 | 2.11 | 4 | â | â | â | â |
| Hao et al. | 2022 | â | 2.88 | â | 4 | 0.537 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Liu et al. (2025)
Classified as primordial binary cluster 311 along with DBSB_19, and of multiple system 23 along with DBSB_19, CWNU_102 and Pismis_5.
Palma et al. (2025)
Part of multiple system G68, along with Pismis_5, CWNU_102 and DBSB_19.
Cavallo et al. (2024)
Gold sample.