UPK 18
0.66
UTI
0.41
CN
1.0
Cdens
0.5
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
8.8 [arcmin]
- CN 0.41 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 18 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Close
Moderate 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 | 280.784 | -15.325 | 1.291 | 3.062 | 0.866 | -20.594 |
| Li et al. | 2025 | 280.763 | -15.325 | 1.28 | 3.112 | 0.98 | â |
| Almeida et al. | 2025 | 280.759 | -15.308 | â | â | â | â |
| Alfonso et al. | 2024 | 280.698 | -15.283 | 1.242 | 2.972 | 0.792 | â |
| Hunt & Reffert | 2024 | 280.771 | -15.317 | 1.307 | 3.002 | 0.839 | -16.58 |
| Cavallo et al. | 2024 | 280.754 | -15.328 | 1.301 | â | â | â |
| Hunt & Reffert | 2023 | 280.771 | -15.317 | 1.307 | 3.002 | 0.839 | -16.58 |
| Almeida et al. | 2023 | 280.747 | -15.305 | â | â | â | â |
| Dias et al. | 2021 | 280.759 | -15.308 | 1.266 | 3.075 | 0.92 | â |
| Cantat-Gaudin et al. | 2020 | 280.763 | -15.325 | 1.28 | 3.112 | 0.98 | â |
| Cantat-Gaudin & Anders | 2020 | 280.761 | -15.33 | 1.243 | 3.102 | 0.934 | â |
| Sim et al. | 2019 | 280.771 | -15.304 | â | 3.08 | 0.87 | 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 | 1.02 | 1.26 | â | 665 | 0.040 | â | â | â |
| Almeida et al. | 2025 | 0.81 | 1.41 | â | 154 | â | 137 | â | â |
| Alfonso et al. | 2024 | 0.78 | 1.04 | â | 75 | 0.032 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 109* | â | â |
| Cavallo et al. | 2024 | 0.75 | 1.11 | â | 380 | -0.310 | â | â | â |
| Hunt & Reffert | 2023 | 0.74 | 1.11 | 0.83 | 350 | â | â | â | â |
| Almeida et al. | 2023 | 0.75 | 1.03 | â | 614 | -0.228 | 102* | 0.75 | â |
| Tarricq et al. | 2022 | 0.76 | â | â | 724 | â | â | â | â |
| Dias et al. | 2021 | 0.81 | 1.41 | â | 154 | 0.032 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.78 | 1.04 | â | 724 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.79 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.75 | â | â | 282 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.