UPK 436
0.69
UTI
0.74
CN
0.58
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
23.8 [arcmin]
- CN 0.74 Moderately populated
- Cdens 0.58 Moderately dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 436 is a moderately populated, moderately 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 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 | 100.211 | -8.091 | 1.18 | -4.093 | 0.636 | 23.968 |
| Li et al. | 2025 | 100.18 | -8.126 | 1.157 | -4.119 | 0.635 | â |
| Almeida et al. | 2025 | 100.18 | -8.166 | â | â | â | â |
| Alfonso et al. | 2024 | 100.28 | -8.156 | 1.151 | -4.098 | 0.654 | â |
| Hunt & Reffert | 2024 | 100.328 | -7.998 | 1.183 | -4.131 | 0.649 | 18.709 |
| Celli et al. | 2024 | 100.18 | -8.126 | â | â | â | â |
| Cavallo et al. | 2024 | 100.113 | -8.126 | 1.186 | â | â | â |
| Hunt & Reffert | 2023 | 100.328 | -7.998 | 1.183 | -4.131 | 0.649 | 18.709 |
| Almeida et al. | 2023 | 100.179 | -8.178 | â | â | â | â |
| Dias et al. | 2021 | 100.18 | -8.166 | 1.168 | -4.159 | 0.645 | 24.886 |
| Cantat-Gaudin et al. | 2020 | 100.18 | -8.126 | 1.157 | -4.119 | 0.635 | â |
| Cantat-Gaudin & Anders | 2020 | 100.2 | -8.097 | 1.167 | -4.17 | 0.607 | â |
| Sim et al. | 2019 | 100.231 | -8.128 | â | -4.1 | 0.66 | 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 | 0.38 | â | 27 | -0.259 | â | â | â |
| Almeida et al. | 2025 | 0.82 | 0.48 | â | 62 | â | 244 | â | â |
| Alfonso et al. | 2024 | 0.85 | 0.23 | â | 20 | 0.049 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 117* | â | â |
| Celli et al. | 2024 | â | â | â | 26 | â | 337 | â | â |
| Cavallo et al. | 2024 | 0.87 | 0.48 | â | 9 | -0.020 | â | â | â |
| Hunt & Reffert | 2023 | 0.80 | 0.21 | 0.84 | 15 | â | â | â | â |
| Almeida et al. | 2023 | 0.81 | 0.47 | â | 53 | -0.003 | 328* | 0.69 | â |
| Dias et al. | 2021 | 0.82 | 0.48 | â | 62 | 0.049 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.85 | 0.23 | â | 26 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.84 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.84 | â | â | 20 | 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.