UPK 16
0.70
UTI
0.5
CN
0.84
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
14.8 [arcmin]
- CN 0.5 Moderately populated
- Cdens 0.84 Dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 16 is a moderately populated, dense 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, young cluster, but with a large variance across recent sources for the absorption, age, and metallicity parameters (see Parameters). It is moderately studied in the literature.
Close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 287.29 | -19.101 | 1.238 | -0.376 | -5.173 | 4.837 |
| Li et al. | 2025 | 287.36 | -19.11 | 1.196 | -0.428 | -5.166 | â |
| Hu & Soubiran | 2025 | 287.298 | -19.07 | â | â | â | â |
| Almeida et al. | 2025 | 287.222 | -19.106 | â | â | â | â |
| Hunt & Reffert | 2024 | 287.366 | -19.069 | 1.214 | -0.38 | -5.149 | 0.968 |
| Cavallo et al. | 2024 | 287.298 | -19.07 | 1.226 | â | â | â |
| Hunt & Reffert | 2023 | 287.366 | -19.069 | 1.214 | -0.38 | -5.149 | 0.968 |
| Almeida et al. | 2023 | 287.225 | -19.13 | â | â | â | â |
| He et al. | 2022 | 287.324 | -19.093 | 1.27 | -0.309 | -5.135 | â |
| Dias et al. | 2021 | 287.222 | -19.106 | 1.221 | -0.416 | -5.132 | 13.566 |
| Cantat-Gaudin et al. | 2020 | 287.36 | -19.11 | 1.196 | -0.428 | -5.166 | â |
| Cantat-Gaudin & Anders | 2020 | 287.264 | -19.102 | 1.216 | -0.398 | -5.11 | â |
| Sim et al. | 2019 | 287.268 | -19.08 | â | -0.4 | -5.14 | 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 | 0.72 | 0.52 | â | 100 | -0.215 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.130* | â | â | â |
| Almeida et al. | 2025 | 0.79 | 0.60 | â | 86 | â | 64 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 141* | â | â |
| Cavallo et al. | 2024 | 0.82 | 0.00 | â | 617 | 0.800 | â | â | â |
| Hunt & Reffert | 2023 | 0.78 | 0.37 | 0.84 | 229 | â | â | â | â |
| Almeida et al. | 2023 | 0.79 | 0.48 | â | 221 | -0.104 | 129* | 0.66 | â |
| He et al. | 2022 | â | 0.55 | â | 71 | â | â | â | â |
| Dias et al. | 2021 | 0.79 | 0.60 | â | 86 | 0.023 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.80 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.80 | 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.