UPK 467
0.85
UTI
0.76
CN
0.97
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
31.4 [arcmin]
- CN 0.76 Rich
- Cdens 0.97 Very dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 467 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, above 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 absorption parameter (see Parameters). It is well-studied in the literature.
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 | 121.259 | -11.42 | 1.7 | -6.949 | -1.633 | 15.424 |
| Li et al. | 2025 | 121.237 | -11.42 | 1.692 | -6.968 | -1.662 | â |
| Almeida et al. | 2025 | 121.209 | -11.478 | â | â | â | â |
| Alfonso et al. | 2024 | 121.211 | -11.399 | 1.659 | -6.912 | -1.61 | â |
| Hunt & Reffert | 2024 | 121.29 | -11.325 | 1.69 | -6.932 | -1.566 | 18.897 |
| Cavallo et al. | 2024 | 121.118 | -11.485 | 1.691 | â | â | â |
| Hunt & Reffert | 2023 | 121.29 | -11.325 | 1.69 | -6.932 | -1.566 | 18.897 |
| Almeida et al. | 2023 | 121.152 | -11.555 | â | â | â | â |
| He et al. | 2022 | 121.295 | -11.423 | 1.709 | -6.949 | -1.622 | â |
| Tarricq et al. | 2022 | 121.391 | -11.306 | 1.738 | -6.929 | -1.62 | â |
| Dias et al. | 2021 | 121.209 | -11.478 | 1.703 | -6.948 | -1.653 | 19.461 |
| Cantat-Gaudin et al. | 2020 | 121.237 | -11.42 | 1.692 | -6.968 | -1.662 | â |
| Cantat-Gaudin & Anders | 2020 | 121.237 | -11.416 | 1.704 | -6.975 | -1.653 | â |
| Sim et al. | 2019 | 121.251 | -11.437 | â | -6.99 | -1.72 | 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 | 0.59 | 0.11 | â | 139 | 0.048 | â | â | â |
| Almeida et al. | 2025 | 0.59 | 0.25 | â | 149 | â | 189 | â | â |
| Alfonso et al. | 2024 | 0.58 | 0.13 | â | 101 | -0.083 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 115* | â | â |
| Cavallo et al. | 2024 | 0.57 | 0.25 | â | 234 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 0.56 | 0.10 | 0.74 | 131 | â | â | â | â |
| Almeida et al. | 2023 | 0.57 | 0.01 | â | 100 | -0.045 | 227* | 0.47 | â |
| He et al. | 2022 | â | 0.05 | â | 282 | â | â | â | â |
| Tarricq et al. | 2022 | 0.57 | â | â | 123 | â | â | â | â |
| Dias et al. | 2021 | 0.59 | 0.25 | â | 149 | -0.083 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.58 | 0.13 | â | 117 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.58 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.58 | â | â | 158 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.