UBC 622
0.06
UTI
0.0
CN
0.06
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
8.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
UBC 622 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Distant
Low extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 111.79 | 9.299 | 0.279 | -1.215 | 0.185 | 88.928 |
| Li et al. | 2025 | 111.743 | 9.299 | 0.288 | -1.081 | 0.169 | â |
| Cantat-Gaudin et al. | 2020 | 111.743 | 9.299 | 0.288 | -1.081 | 0.169 | â |
| Castro-Ginard et al. | 2020 | 111.733 | 9.253 | 0.277 | -1.111 | 0.189 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 4.35 | 0.37 | â | 2152 | -0.349 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.28 | 0.41 | â | 759 | â | â | â | â |

