UPK 136
0.60
UTI
0.58
CN
0.27
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
1.3 [N/pc2]
- CN 0.58 Moderately populated
- Cdens 0.27 Loose
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 136 is a moderately populated, loose 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, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 322.786 | 43.476 | 1.549 | 0.013 | -0.627 | -8.332 |
| Li et al. | 2025 | 322.841 | 43.441 | 1.533 | 0.012 | -0.591 | â |
| Almeida et al. | 2025 | 322.741 | 43.466 | â | â | â | â |
| Alfonso et al. | 2024 | 322.611 | 43.356 | 1.499 | -0.03 | -0.617 | â |
| Zhang et al. | 2024 | 322.609 | 43.417 | â | â | â | â |
| Hunt & Reffert | 2024 | 322.609 | 43.417 | 1.564 | -0.001 | -0.666 | -5.349 |
| Cavallo et al. | 2024 | 322.712 | 43.395 | 1.557 | â | â | â |
| Hunt & Reffert | 2023 | 322.609 | 43.417 | 1.564 | -0.001 | -0.666 | -5.349 |
| Tarricq et al. | 2022 | 322.75 | 43.491 | 1.522 | 0.041 | -0.656 | â |
| Dias et al. | 2021 | 322.741 | 43.466 | 1.532 | 0.034 | -0.592 | -2.866 |
| Cantat-Gaudin et al. | 2020 | 322.841 | 43.441 | 1.533 | 0.012 | -0.591 | â |
| Cantat-Gaudin & Anders | 2020 | 322.828 | 43.491 | 1.52 | 0.022 | -0.587 | â |
| Sim et al. | 2019 | 322.602 | 43.339 | â | -0.03 | -0.6 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.64 | 0.36 | 0.59 | 130 | -0.075 | 96 | â | â |
| Liu et al. | 2025 | 0.74 | 0.10 | â | 417 | â | â | â | â |
| Li et al. | 2025 | 0.67 | 0.42 | â | 125 | -0.035 | â | â | â |
| Almeida et al. | 2025 | 0.65 | 0.43 | â | 143 | â | 150 | â | â |
| Alfonso et al. | 2024 | 0.63 | 0.31 | â | 95 | -0.075 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.205(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 42(1) | â | â |
| Cavallo et al. | 2024 | 0.63 | 0.41 | â | 245 | 0.110 | â | â | â |
| Hunt & Reffert | 2023 | 0.62 | 0.20 | 0.59 | 136 | â | â | â | â |
| Tarricq et al. | 2022 | 0.61 | â | â | 123 | â | â | â | â |
| Dias et al. | 2021 | 0.65 | 0.43 | â | 143 | -0.075 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.63 | 0.31 | â | 115 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.65 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.64 | â | â | 71 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 170 along with HSC_689.
Palma et al. (2025)
Part of multiple system G190, along with HSC_689, HSC_717 and HSC_699.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.