UPK 219
0.57
UTI
0.29
CN
0.51
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Stellar density (N50/rad)
2.6 [N/pc2]
- CN 0.29 Poorly populated
- Cdens 0.51 Moderately dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 219 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 352.048 | 65.35 | 1.216 | -1.76 | -2.549 | -6.939 |
| Li et al. | 2025 | 351.854 | 65.31 | 1.21 | -1.734 | -2.459 | â |
| Almeida et al. | 2025 | 351.839 | 65.275 | â | â | â | â |
| Alfonso et al. | 2024 | -8.305 | 65.346 | 1.189 | -1.771 | -2.546 | â |
| Hunt & Reffert | 2024 | 352.012 | 65.377 | 1.219 | -1.778 | -2.551 | -7.048 |
| Cavallo et al. | 2024 | 351.96 | 65.341 | 1.215 | â | â | â |
| Hunt & Reffert | 2023 | 352.012 | 65.377 | 1.219 | -1.778 | -2.551 | -7.048 |
| Almeida et al. | 2023 | 351.763 | 65.253 | â | â | â | â |
| Dias et al. | 2021 | 351.839 | 65.275 | 1.195 | -1.747 | -2.471 | â |
| Cantat-Gaudin et al. | 2020 | 351.854 | 65.31 | 1.21 | -1.734 | -2.459 | â |
| Cantat-Gaudin & Anders | 2020 | 351.854 | 65.303 | 1.202 | -1.751 | -2.465 | â |
| Sim et al. | 2019 | 351.781 | 65.304 | â | -1.72 | -2.48 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.8 | 1.485 | 0.77 | 206 | 0.054 | 92 | 0.71 | â |
| Li et al. | 2025 | 0.72 | 1.39 | â | 251 | 0.054 | â | â | â |
| Almeida et al. | 2025 | 0.79 | 1.49 | â | 211 | â | 77 | â | â |
| Alfonso et al. | 2024 | 0.87 | 1.20 | â | 342 | 0.008 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 92(1) | â | â |
| Cavallo et al. | 2024 | 0.78 | 1.48 | â | 200 | 0.280 | â | â | â |
| Hunt & Reffert | 2023 | 0.80 | 1.53 | 0.77 | 144 | â | â | â | â |
| Almeida et al. | 2023 | 0.80 | 1.52 | â | 202 | 0.104 | 96(1) | 0.71 | â |
| Tarricq et al. | 2022 | 0.85 | â | â | 166 | â | â | â | â |
| Dias et al. | 2021 | 0.79 | 1.49 | â | 211 | 0.008 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.87 | 1.20 | â | 148 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.81 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.80 | â | â | 794 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P586, along with Theia_667.
Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg59' along with UPK 220.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.