UPK 46
0.65
UTI
0.5
CN
0.6
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
20.6 [arcmin]
- CN 0.5 Moderately populated
- Cdens 0.6 Moderately dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 46 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, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately 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 | 294.612 | -1.367 | 1.458 | 0.127 | -8.562 | 0.46 |
| Li et al. | 2025 | 294.707 | -1.363 | 1.47 | 0.094 | -8.631 | â |
| Almeida et al. | 2025 | 294.709 | -1.356 | â | â | â | â |
| Alfonso et al. | 2024 | 294.542 | -1.437 | 1.416 | 0.136 | -8.57 | â |
| Hunt & Reffert | 2024 | 294.626 | -1.312 | 1.457 | 0.141 | -8.612 | 0.718 |
| Cavallo et al. | 2024 | 294.441 | -1.72 | 1.459 | â | â | â |
| Hunt & Reffert | 2023 | 294.626 | -1.312 | 1.457 | 0.141 | -8.612 | 0.718 |
| Almeida et al. | 2023 | 294.718 | -1.33 | â | â | â | â |
| Tarricq et al. | 2022 | 294.531 | -1.411 | 1.465 | 0.119 | -8.627 | â |
| Dias et al. | 2021 | 294.709 | -1.356 | 1.473 | 0.063 | -8.726 | â |
| Cantat-Gaudin et al. | 2020 | 294.707 | -1.363 | 1.47 | 0.094 | -8.631 | â |
| Cantat-Gaudin & Anders | 2020 | 294.7 | -1.365 | 1.473 | 0.071 | -8.729 | â |
| Sim et al. | 2019 | 294.622 | -1.358 | â | 0.11 | -8.6 | 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 | 0.71 | 1.02 | â | 88 | -0.253 | â | â | â |
| Almeida et al. | 2025 | 0.67 | 0.98 | â | 139 | â | 105 | â | â |
| Alfonso et al. | 2024 | 0.69 | 0.64 | â | 208 | 0.069 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 50* | â | â |
| Cavallo et al. | 2024 | 0.65 | 0.77 | â | 251 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 0.64 | 0.80 | 0.91 | 104 | â | â | â | â |
| Almeida et al. | 2023 | 0.67 | 0.79 | â | 292 | 0.025 | 144* | 0.64 | â |
| Tarricq et al. | 2022 | 0.68 | â | â | 162 | â | â | â | â |
| Dias et al. | 2021 | 0.67 | 0.98 | â | 139 | 0.069 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.69 | 0.64 | â | 155 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.67 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.68 | â | â | 79 | 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.