UBC 36
0.60
UTI
0.3
CN
1.0
Cdens
0.5
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
3.5 [arcmin]
- CN 0.3 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 36 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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 metallicity parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a large 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 | 16.486 | 59.628 | 0.496 | -1.156 | -0.451 | -51.505 |
| Li et al. | 2025 | 16.487 | 59.632 | 0.471 | -1.166 | -0.406 | â |
| Almeida et al. | 2025 | 16.456 | 59.635 | â | â | â | â |
| Hunt & Reffert | 2024 | 16.463 | 59.63 | 0.476 | -1.201 | -0.489 | -51.507 |
| Cavallo et al. | 2024 | 16.38 | 59.636 | 0.478 | â | â | â |
| Hunt & Reffert | 2023 | 16.463 | 59.63 | 0.476 | -1.201 | -0.489 | -51.507 |
| Almeida et al. | 2023 | 16.446 | 59.633 | â | â | â | â |
| Dias et al. | 2021 | 16.456 | 59.635 | 0.405 | -1.183 | -0.472 | -50.455 |
| Cantat-Gaudin et al. | 2020 | 16.487 | 59.632 | 0.471 | -1.166 | -0.406 | â |
| Cantat-Gaudin & Anders | 2020 | 16.487 | 59.632 | 0.471 | -1.166 | -0.406 | â |
| Castro-Ginard et al. | 2019 | 16.47 | 59.638 | 0.466 | -1.213 | -0.462 | 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 | 1.73 | 1.19 | â | 541 | -0.049 | â | â | â |
| Almeida et al. | 2025 | 1.90 | 1.48 | â | 270 | â | 211 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 179* | â | â |
| Cavallo et al. | 2024 | 1.99 | 1.46 | â | 229 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 1.89 | 1.13 | 0.94 | 324 | â | â | â | â |
| Almeida et al. | 2023 | 1.75 | 1.34 | â | 478 | -0.070 | 107* | 0.44 | â |
| Dias et al. | 2021 | 1.90 | 1.48 | â | 270 | -0.097 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.04 | 1.00 | â | 537 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.00 | â | â | â | 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.