UPK 594
0.52
UTI
0.33
CN
0.22
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
19.7 [arcmin]
- CN 0.33 Poorly populated
- Cdens 0.22 Very loose
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 594 is a poorly populated, very loose object of 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, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately 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 | 218.941 | -67.999 | 1.052 | -1.947 | -3.108 | 0.214 |
| Li et al. | 2025 | 219.173 | -67.975 | 1.029 | -1.9 | -3.118 | â |
| Almeida et al. | 2025 | 218.608 | -68.005 | â | â | â | â |
| Alfonso et al. | 2024 | 219.153 | -67.844 | 1.017 | -2.091 | -3.147 | â |
| Hunt & Reffert | 2024 | 218.776 | -67.937 | 1.045 | -2.053 | -3.126 | -0.111 |
| Cavallo et al. | 2024 | 218.836 | -67.962 | 1.048 | â | â | â |
| Hunt & Reffert | 2023 | 218.776 | -67.937 | 1.045 | -2.053 | -3.126 | -0.111 |
| Tarricq et al. | 2022 | 219.351 | -68.053 | 1.068 | -1.893 | -3.108 | â |
| Dias et al. | 2021 | 218.608 | -68.005 | 1.037 | -2.001 | -3.095 | â |
| Cantat-Gaudin et al. | 2020 | 219.173 | -67.975 | 1.029 | -1.9 | -3.118 | â |
| Cantat-Gaudin & Anders | 2020 | 218.738 | -67.996 | 1.029 | -1.975 | -3.129 | â |
| Sim et al. | 2019 | 218.917 | -67.966 | â | -1.98 | -3.16 | 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 | 1.08 | 0.92 | â | 77 | 0.148 | â | â | â |
| Almeida et al. | 2025 | 0.95 | 0.94 | â | 324 | â | 134 | â | â |
| Alfonso et al. | 2024 | 0.94 | 0.81 | â | 74 | 0.113 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 111* | â | â |
| Cavallo et al. | 2024 | 0.92 | 0.74 | â | 417 | 0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.91 | 0.72 | 1.11 | 104 | â | â | â | â |
| Tarricq et al. | 2022 | 0.91 | â | â | 155 | â | â | â | â |
| Dias et al. | 2021 | 0.95 | 0.94 | â | 324 | 0.113 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.94 | 0.81 | â | 151 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.95 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.94 | â | â | 79 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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