UBC 1246
0.45
UTI
0.55
CN
0.43
Cdens
0.5
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
6.2 [arcmin]
- CN 0.55 Moderately populated
- Cdens 0.43 Loose
- CC3 0.5 Intermediate quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1246 is a moderately populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 45.483 | 47.959 | 0.34 | 0.528 | -1.235 | -28.68 |
| Hu & Soubiran | 2025 | 45.464 | 47.958 | â | â | â | â |
| Zhang et al. | 2024 | 45.52 | 47.974 | â | â | â | â |
| Hunt & Reffert | 2024 | 45.52 | 47.974 | 0.335 | 0.502 | -1.232 | -34.657 |
| Cavallo et al. | 2024 | 45.464 | 47.957 | 0.335 | â | â | â |
| Hunt & Reffert | 2023 | 45.52 | 47.974 | 0.335 | 0.502 | -1.232 | -34.657 |
| Castro-Ginard et al. | 2022 | 45.47 | 47.94 | 0.34 | 0.53 | -1.26 | -36.9 |
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 | -0.110* | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.085* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 426* | â | â |
| Cavallo et al. | 2024 | 2.41 | 1.27 | â | 1023 | -0.220 | â | â | â |
| Hunt & Reffert | 2023 | 2.58 | 0.63 | 1.07 | 879 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 3.10 | 0.83 | â | 1012 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.