UPK 567
0.77
UTI
0.6
CN
0.72
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
23.7 [arcmin]
- CN 0.6 Moderately populated
- Cdens 0.72 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 567 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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 | 161.049 | -67.549 | 1.558 | -6.368 | 0.107 | 5.909 |
| Li et al. | 2025 | 161.029 | -67.524 | 1.538 | -6.374 | 0.109 | â |
| Hu & Soubiran | 2025 | 160.935 | -67.407 | â | â | â | â |
| Almeida et al. | 2025 | 161.146 | -67.46 | â | â | â | â |
| Alfonso et al. | 2024 | 161.097 | -67.552 | 1.524 | -6.378 | 0.129 | â |
| Hunt & Reffert | 2024 | 160.951 | -67.52 | 1.561 | -6.403 | 0.197 | 6.946 |
| Cavallo et al. | 2024 | 160.934 | -67.407 | 1.558 | â | â | â |
| Hunt & Reffert | 2023 | 160.951 | -67.52 | 1.561 | -6.403 | 0.197 | 6.946 |
| Almeida et al. | 2023 | 161.706 | -67.299 | â | â | â | â |
| Tarricq et al. | 2022 | 161.159 | -67.576 | 1.54 | -6.367 | 0.112 | â |
| Dias et al. | 2021 | 161.146 | -67.46 | 1.547 | -6.347 | 0.114 | 4.889 |
| Cantat-Gaudin et al. | 2020 | 161.029 | -67.524 | 1.538 | -6.374 | 0.109 | â |
| Cantat-Gaudin & Anders | 2020 | 161.024 | -67.505 | 1.536 | -6.363 | 0.101 | â |
| Sim et al. | 2019 | 161.064 | -67.53 | â | -6.37 | 0.11 | 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 | 0.63 | 0.56 | â | 439 | -0.038 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.120* | â | â | â |
| Almeida et al. | 2025 | 0.64 | 0.62 | â | 448 | â | 101 | â | â |
| Alfonso et al. | 2024 | 0.65 | 0.47 | â | 489 | -0.015 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 49* | â | â |
| Cavallo et al. | 2024 | 0.63 | 0.68 | â | 741 | 0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.62 | 0.43 | 1.04 | 411 | â | â | â | â |
| Almeida et al. | 2023 | 0.63 | 0.69 | â | 456 | -0.054 | 149* | 0.58 | â |
| Tarricq et al. | 2022 | 0.64 | â | â | 363 | â | â | â | â |
| Dias et al. | 2021 | 0.64 | 0.62 | â | 448 | -0.015 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.65 | 0.47 | â | 339 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.64 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.64 | â | â | 501 | 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.