UPK 26
0.62
UTI
0.52
CN
0.52
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
17.1 [arcmin]
- CN 0.52 Moderately populated
- Cdens 0.52 Moderately dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 26 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 (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 | 283.465 | -9.808 | 1.089 | 0.08 | -4.451 | 2.642 |
| Li et al. | 2025 | 283.438 | -9.847 | 1.108 | 0.062 | -4.419 | â |
| Almeida et al. | 2025 | 283.472 | -9.8 | â | â | â | â |
| Alfonso et al. | 2024 | 283.722 | -9.474 | 1.036 | 0.078 | -4.382 | â |
| Hunt & Reffert | 2024 | 283.472 | -9.831 | 1.083 | 0.097 | -4.41 | 3.525 |
| Cavallo et al. | 2024 | 283.526 | -9.751 | 1.088 | â | â | â |
| Hunt & Reffert | 2023 | 283.472 | -9.831 | 1.083 | 0.097 | -4.41 | 3.525 |
| Tarricq et al. | 2022 | 283.494 | -9.77 | 1.094 | 0.11 | -4.452 | â |
| Dias et al. | 2021 | 283.472 | -9.8 | 1.113 | 0.056 | -4.406 | â |
| Cantat-Gaudin et al. | 2020 | 283.438 | -9.847 | 1.108 | 0.062 | -4.419 | â |
| Cantat-Gaudin & Anders | 2020 | 283.451 | -9.796 | 1.108 | 0.067 | -4.416 | â |
| Sim et al. | 2019 | 283.469 | -9.827 | â | 0.08 | -4.42 | 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 | 0.95 | 0.85 | â | 60 | 0.360 | â | â | â |
| Almeida et al. | 2025 | 0.88 | 1.00 | â | 92 | â | 129 | â | â |
| Alfonso et al. | 2024 | 0.85 | 0.59 | â | 205 | 0.078 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 279* | â | â |
| Cavallo et al. | 2024 | 0.92 | 1.15 | â | 59 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 0.88 | 0.85 | 0.78 | 109 | â | â | â | â |
| Tarricq et al. | 2022 | 0.83 | â | â | 81 | â | â | â | â |
| Dias et al. | 2021 | 0.88 | 1.00 | â | 92 | 0.078 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.86 | 0.59 | â | 72 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.88 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.88 | â | â | 112 | 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.