UPK 433
0.39
UTI
0.62
CN
0.93
Cdens
0.75
CC3
0.56
Clit
0.57
Cdup
Stellar density (N50/rad)
4.6 [N/pc2]
- CN 0.62 Moderately populated
- Cdens 0.93 Very dense
- CC3 0.75 High quality
- Clit 0.56 Moderately studied
- Cdup 0.57 Likely unique
Overview
UPK 433 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously 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 | 103.38 | -5.691 | 1.267 | -0.763 | -2.522 | 23.176 |
| Li et al. | 2025 | 103.455 | -5.729 | 1.248 | -0.783 | -2.527 | â |
| Almeida et al. | 2025 | 103.457 | -5.763 | â | â | â | â |
| Alfonso et al. | 2024 | 103.397 | -5.656 | 1.232 | -0.763 | -2.503 | â |
| Almeida et al. | 2023 | 103.437 | -5.815 | â | â | â | â |
| He et al. | 2022 | 103.317 | -5.67 | 1.274 | -0.784 | -2.523 | â |
| Tarricq et al. | 2022 | 103.444 | -5.646 | 1.278 | -0.743 | -2.526 | â |
| Dias et al. | 2021 | 103.457 | -5.763 | 1.246 | -0.774 | -2.48 | 22.002 |
| Cantat-Gaudin et al. | 2020 | 103.455 | -5.729 | 1.248 | -0.783 | -2.527 | â |
| Cantat-Gaudin & Anders | 2020 | 103.424 | -5.656 | 1.247 | -0.765 | -2.477 | â |
| Sim et al. | 2019 | 103.382 | -5.739 | â | -0.78 | -2.55 | 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 | 0.77 | 0.32 | â | 334 | -0.003 | 150 | 0.47 | â |
| Li et al. | 2025 | 0.74 | 0.16 | â | 532 | -0.046 | â | â | â |
| Almeida et al. | 2025 | 0.76 | 0.32 | â | 334 | â | 91 | â | â |
| Alfonso et al. | 2024 | 0.79 | 0.25 | â | 357 | 0.041 | â | â | â |
| Almeida et al. | 2023 | 0.76 | 0.38 | â | 384 | -0.055 | 209(1) | 0.47 | â |
| He et al. | 2022 | â | 0.50 | â | 200 | â | â | â | â |
| Tarricq et al. | 2022 | 0.77 | â | â | 204 | â | â | â | â |
| Dias et al. | 2021 | 0.76 | 0.32 | â | 334 | 0.041 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.79 | 0.25 | â | 182 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.78 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.78 | â | â | 79 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.