UBC 56
(FoF 2230)
0.79
UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
15.4 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 56 is a rich, very dense object of high C3 quality. Its parallax locates it at a 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 moderate percentage of members with a later reported entry. See table with shared members information.
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 | 69.867 | 47.542 | 1.137 | 1.502 | -4.069 | -4.489 |
| Li et al. | 2025 | 69.874 | 47.534 | 1.118 | 1.594 | -4.008 | â |
| Alfonso et al. | 2024 | 69.832 | 47.498 | 1.084 | 1.529 | -4.102 | â |
| Zhang et al. | 2024 | 69.868 | 47.564 | â | â | â | â |
| Hunt & Reffert | 2024 | 69.868 | 47.564 | 1.135 | 1.51 | -4.07 | -5.254 |
| Cavallo et al. | 2024 | 69.829 | 47.504 | 1.134 | â | â | â |
| Hunt & Reffert | 2023 | 69.868 | 47.564 | 1.135 | 1.51 | -4.07 | -5.254 |
| He et al. | 2022 | 69.89 | 47.486 | 1.146 | 1.5 | -4.073 | â |
| Tarricq et al. | 2022 | 69.86 | 47.534 | 1.159 | 1.506 | -4.077 | â |
| Cantat-Gaudin et al. | 2020 | 69.874 | 47.534 | 1.118 | 1.594 | -4.008 | â |
| Cantat-Gaudin & Anders | 2020 | 69.874 | 47.534 | 1.118 | 1.594 | -4.008 | â |
| Liu & Pang | 2019 | 69.869 | 47.518 | 1.12 | 1.605 | -4.022 | â |
| Castro-Ginard et al. | 2019 | 69.877 | 47.527 | 1.112 | 1.618 | -4.007 | 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 | 0.76 | 1.89 | â | 422 | -0.136 | â | â | â |
| Alfonso et al. | 2024 | 0.89 | 1.59 | â | 402 | -0.053 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.230* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 675* | â | â |
| Cavallo et al. | 2024 | 0.95 | 1.87 | â | 398 | 0.590 | â | â | â |
| Hunt & Reffert | 2023 | 0.83 | 1.99 | 1.77 | 274 | â | â | â | â |
| He et al. | 2022 | â | 2.40 | â | 56 | â | â | â | â |
| Tarricq et al. | 2022 | 0.87 | â | â | 617 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.89 | 1.59 | â | 603 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.87 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 355 | 0.250 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.