UBC 1133
0.62
UTI
0.73
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
3.6 [arcmin]
- CN 0.73 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1133 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high 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 poorly studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Relatively close
High 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 | 314.587 | 49.91 | 0.398 | -3.498 | -7.165 | -34.623 |
| Hu & Soubiran | 2025 | 314.58 | 49.876 | â | â | â | â |
| Hunt & Reffert | 2024 | 314.584 | 49.911 | 0.409 | -3.497 | -7.155 | -33.931 |
| Cavallo et al. | 2024 | 314.58 | 49.876 | 0.402 | â | â | â |
| Hunt & Reffert | 2023 | 314.584 | 49.911 | 0.409 | -3.497 | -7.155 | -33.931 |
| Castro-Ginard et al. | 2022 | 314.6 | 49.9 | 0.39 | -3.51 | -7.15 | -33.74 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | 0.000* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 845* | â | â |
| Cavallo et al. | 2024 | 2.29 | 3.41 | â | 1148 | 0.360 | â | â | â |
| Hunt & Reffert | 2023 | 2.38 | 3.59 | 1.60 | 865 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 2.63 | 2.93 | â | 895 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.