UPK 155
0.50
UTI
0.31
CN
0.3
Cdens
0.5
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
17.0 [arcmin]
- CN 0.31 Poorly populated
- Cdens 0.3 Loose
- CC3 0.5 Intermediate quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 155 is a poorly populated, loose object of intermediate 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 metallicity 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 | 311.475 | 60.913 | 1.091 | -2.217 | -3.9 | -19.354 |
| Li et al. | 2025 | 311.731 | 60.867 | 1.096 | -2.255 | -3.856 | â |
| Almeida et al. | 2025 | 311.719 | 60.796 | â | â | â | â |
| Alfonso et al. | 2024 | 311.322 | 60.643 | 1.078 | -2.575 | -3.918 | â |
| Hunt & Reffert | 2024 | 311.237 | 60.748 | 1.09 | -2.2 | -3.877 | -20.757 |
| Cavallo et al. | 2024 | 311.623 | 60.883 | 1.091 | â | â | â |
| Hunt & Reffert | 2023 | 311.237 | 60.748 | 1.09 | -2.2 | -3.877 | -20.757 |
| Almeida et al. | 2023 | 311.706 | 60.744 | â | â | â | â |
| Dias et al. | 2021 | 311.719 | 60.796 | 1.099 | -2.268 | -3.862 | â |
| Cantat-Gaudin et al. | 2020 | 311.731 | 60.867 | 1.096 | -2.255 | -3.856 | â |
| Cantat-Gaudin & Anders | 2020 | 311.656 | 60.867 | 1.089 | -2.293 | -3.904 | â |
| Sim et al. | 2019 | 311.706 | 60.901 | â | -2.24 | -3.86 | 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 | 0.83 | 1.00 | â | 201 | -0.141 | â | â | â |
| Almeida et al. | 2025 | 0.88 | 1.17 | â | 72 | â | 69 | â | â |
| Alfonso et al. | 2024 | 0.84 | 0.69 | â | 224 | 0.011 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 51* | â | â |
| Cavallo et al. | 2024 | 0.92 | 1.00 | â | 58 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 0.86 | 0.97 | 0.81 | 46 | â | â | â | â |
| Almeida et al. | 2023 | 0.87 | 1.25 | â | 157 | 0.002 | 260* | 0.66 | â |
| Tarricq et al. | 2022 | 0.82 | â | â | 229 | â | â | â | â |
| Dias et al. | 2021 | 0.88 | 1.17 | â | 72 | 0.010 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.84 | 0.69 | â | 214 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.89 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.89 | â | â | 35 | 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.