UBC 113
0.71
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
4.0 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 113 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (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
Moderate extinction
Massive
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 | 285.135 | -1.563 | 0.4 | 0.533 | -0.513 | -1.851 |
| Li et al. | 2025 | 285.138 | -1.557 | 0.386 | 0.499 | -0.512 | â |
| Hunt & Reffert | 2024 | 285.141 | -1.559 | 0.405 | 0.543 | -0.534 | -15.93 |
| Cavallo et al. | 2024 | 285.134 | -1.553 | 0.407 | â | â | â |
| Hunt & Reffert | 2023 | 285.141 | -1.559 | 0.405 | 0.543 | -0.534 | -15.93 |
| Cantat-Gaudin et al. | 2020 | 285.138 | -1.557 | 0.386 | 0.499 | -0.512 | â |
| Castro-Ginard et al. | 2020 | 285.144 | -1.55 | 0.389 | 0.499 | -0.508 | 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 | 1.61 | 1.86 | â | 1085 | -0.059 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1594* | â | â |
| Cavallo et al. | 2024 | 2.23 | 2.52 | â | 457 | 0.150 | â | â | â |
| Hunt & Reffert | 2023 | 2.27 | 2.43 | 1.09 | 415 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.49 | 1.97 | â | 427 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.