UPK 429
0.86
UTI
0.71
CN
1.0
Cdens
1.0
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
12.9 [arcmin]
- CN 0.71 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
UPK 429 is a moderately populated, very dense object of very 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 parameter (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 | 108.92 | -0.833 | 1.135 | -1.976 | 0.079 | 13.983 |
| Li et al. | 2025 | 108.961 | -0.875 | 1.122 | -2.045 | 0.071 | â |
| Almeida et al. | 2025 | 108.962 | -0.929 | â | â | â | â |
| Alfonso et al. | 2024 | 108.899 | -0.833 | 1.064 | -1.952 | 0.097 | â |
| Zhang et al. | 2024 | 108.934 | -0.82 | â | â | â | â |
| Hunt & Reffert | 2024 | 108.934 | -0.82 | 1.117 | -1.94 | 0.095 | 13.436 |
| Cavallo et al. | 2024 | 108.91 | -0.799 | 1.118 | â | â | â |
| Hunt & Reffert | 2023 | 108.934 | -0.82 | 1.117 | -1.94 | 0.095 | 13.436 |
| Almeida et al. | 2023 | 108.942 | -0.989 | â | â | â | â |
| He et al. | 2022 | 108.937 | -0.848 | 1.135 | -1.97 | 0.077 | â |
| Tarricq et al. | 2022 | 108.953 | -0.825 | 1.137 | -1.973 | 0.063 | â |
| Dias et al. | 2021 | 108.962 | -0.929 | 1.122 | -2.102 | 0.095 | 8.805 |
| Cantat-Gaudin et al. | 2020 | 108.961 | -0.875 | 1.122 | -2.045 | 0.071 | â |
| Cantat-Gaudin & Anders | 2020 | 108.961 | -0.884 | 1.124 | -2.066 | 0.083 | â |
| Sim et al. | 2019 | 108.935 | -0.818 | â | -2.01 | 0.07 | 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 | 0.99 | 0.14 | â | 236 | 0.044 | â | â | â |
| Almeida et al. | 2025 | 0.87 | 0.26 | â | 177 | â | 187 | â | â |
| Alfonso et al. | 2024 | 0.90 | 0.09 | â | 150 | -0.020 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.016* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 225* | â | â |
| Cavallo et al. | 2024 | 0.88 | 0.40 | â | 234 | -0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.83 | 0.12 | 0.38 | 168 | â | â | â | â |
| Almeida et al. | 2023 | 0.85 | 0.01 | â | 100 | -0.068 | 362* | 0.60 | â |
| He et al. | 2022 | â | 0.45 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.88 | â | â | 145 | â | â | â | â |
| Dias et al. | 2021 | 0.87 | 0.26 | â | 177 | -0.020 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.90 | 0.09 | â | 141 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.87 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.86 | â | â | 89 | 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.