UPK 431
0.72
UTI
0.5
CN
0.86
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
16.0 [arcmin]
- CN 0.5 Moderately populated
- Cdens 0.86 Dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 431 is a moderately populated, dense object of high 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 absorption and age parameters (see Parameters). It is well-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 | 108.165 | -2.61 | 1.363 | -2.485 | 0.758 | 11.653 |
| Li et al. | 2025 | 108.234 | -2.635 | 1.346 | -2.46 | 0.76 | â |
| Almeida et al. | 2025 | 108.283 | -2.761 | â | â | â | â |
| Alfonso et al. | 2024 | 108.232 | -2.505 | 1.319 | -2.431 | 0.709 | â |
| Hunt & Reffert | 2024 | 108.14 | -2.567 | 1.348 | -2.457 | 0.771 | 7.595 |
| Cavallo et al. | 2024 | 108.167 | -2.726 | 1.356 | â | â | â |
| Hunt & Reffert | 2023 | 108.14 | -2.567 | 1.348 | -2.457 | 0.771 | 7.595 |
| Almeida et al. | 2023 | 108.285 | -2.766 | â | â | â | â |
| He et al. | 2022 | 108.179 | -2.599 | 1.366 | -2.457 | 0.787 | â |
| Tarricq et al. | 2022 | 108.143 | -2.608 | 1.362 | -2.43 | 0.775 | â |
| Dias et al. | 2021 | 108.283 | -2.761 | 1.342 | -2.457 | 0.749 | 17.737 |
| Cantat-Gaudin et al. | 2020 | 108.234 | -2.635 | 1.346 | -2.46 | 0.76 | â |
| Cantat-Gaudin & Anders | 2020 | 108.239 | -2.631 | 1.331 | -2.454 | 0.751 | â |
| Sim et al. | 2019 | 108.186 | -2.721 | â | -2.44 | 0.77 | 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 | 0.91 | 0.17 | â | 212 | -0.057 | â | â | â |
| Almeida et al. | 2025 | 0.73 | 0.25 | â | 233 | â | 166 | â | â |
| Alfonso et al. | 2024 | 0.74 | 0.00 | â | 593 | -0.070 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 136* | â | â |
| Cavallo et al. | 2024 | 0.71 | 0.22 | â | 166 | 0.060 | â | â | â |
| Hunt & Reffert | 2023 | 0.69 | 0.14 | 0.60 | 426 | â | â | â | â |
| Almeida et al. | 2023 | 0.72 | 0.09 | â | 100 | -0.060 | 258* | 0.56 | â |
| He et al. | 2022 | â | 0.30 | â | 178 | â | â | â | â |
| Tarricq et al. | 2022 | 0.75 | â | â | 617 | â | â | â | â |
| Dias et al. | 2021 | 0.73 | 0.25 | â | 233 | -0.073 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.77 | 0.00 | â | 603 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.74 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.73 | â | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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