UBC 1073
0.63
UTI
0.77
CN
0.74
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
5.4 [arcmin]
- CN 0.77 Rich
- Cdens 0.74 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1073 is a rich, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Distant
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 | 298.259 | 30.821 | 0.253 | -1.759 | -3.045 | -24.153 |
| Hu & Soubiran | 2025 | 298.258 | 30.831 | â | â | â | â |
| Hunt & Reffert | 2024 | 298.265 | 30.807 | 0.252 | -1.772 | -3.045 | -20.34 |
| Cavallo et al. | 2024 | 298.258 | 30.831 | 0.253 | â | â | â |
| Hunt & Reffert | 2023 | 298.265 | 30.807 | 0.252 | -1.772 | -3.045 | -20.34 |
| Castro-Ginard et al. | 2022 | 298.25 | 30.81 | 0.25 | -1.77 | -3.04 | -25.62 |
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 | -0.080* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1289* | â | â |
| Cavallo et al. | 2024 | 2.82 | 2.31 | â | 794 | -0.060 | â | â | â |
| Hunt & Reffert | 2023 | 3.57 | 2.43 | 1.81 | 212 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 3.68 | 1.59 | â | 682 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.