UBC 136
0.74
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
8.1 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 136 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate 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.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate 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 | 304.487 | 32.583 | 0.699 | -0.045 | -3.305 | 1.964 |
| Li et al. | 2025 | 304.49 | 32.582 | 0.69 | -0.045 | -3.267 | â |
| Almeida et al. | 2025 | 304.501 | 32.601 | â | â | â | â |
| Hunt & Reffert | 2024 | 304.459 | 32.582 | 0.696 | -0.043 | -3.321 | 4.875 |
| Cavallo et al. | 2024 | 304.504 | 32.599 | 0.695 | â | â | â |
| Hunt & Reffert | 2023 | 304.459 | 32.582 | 0.696 | -0.043 | -3.321 | 4.875 |
| Almeida et al. | 2023 | 304.479 | 32.606 | â | â | â | â |
| Tarricq et al. | 2022 | 304.505 | 32.598 | 0.707 | -0.046 | -3.296 | â |
| Dias et al. | 2021 | 304.501 | 32.601 | 0.693 | -0.028 | -3.261 | â |
| Cantat-Gaudin et al. | 2020 | 304.49 | 32.582 | 0.69 | -0.045 | -3.267 | â |
| Castro-Ginard et al. | 2020 | 304.502 | 32.582 | 0.69 | -0.039 | -3.281 | 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 | 1.02 | 2.13 | â | 468 | 0.052 | â | â | â |
| Almeida et al. | 2025 | 1.38 | 2.51 | â | 140 | â | 557 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1089* | â | â |
| Cavallo et al. | 2024 | 1.58 | 2.79 | â | 68 | 0.390 | â | â | â |
| Hunt & Reffert | 2023 | 1.38 | 2.64 | 1.75 | 105 | â | â | â | â |
| Almeida et al. | 2023 | 1.35 | 2.48 | â | 167 | 0.180 | 710* | 0.71 | â |
| Tarricq et al. | 2022 | 1.32 | â | â | 182 | â | â | â | â |
| Dias et al. | 2021 | 1.38 | 2.51 | â | 140 | 0.297 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.37 | 1.97 | â | 166 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.