UBC 1173
0.50
UTI
0.39
CN
1.0
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
2.3 [arcmin]
- CN 0.39 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1173 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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 metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Distant
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 | 343.314 | 57.014 | 0.255 | -3.015 | -1.012 | -50.564 |
| Hu & Soubiran | 2025 | 343.346 | 57.013 | â | â | â | â |
| Hunt & Reffert | 2024 | 343.321 | 57.018 | 0.251 | -2.989 | -1.012 | -50.568 |
| Cavallo et al. | 2024 | 343.346 | 57.013 | 0.255 | â | â | â |
| Hunt & Reffert | 2023 | 343.321 | 57.018 | 0.251 | -2.989 | -1.012 | -50.568 |
| Castro-Ginard et al. | 2022 | 343.33 | 57.01 | 0.26 | -3.02 | -0.99 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.200* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 341* | â | â |
| Cavallo et al. | 2024 | 3.19 | 1.86 | â | 603 | 0.290 | â | â | â |
| Hunt & Reffert | 2023 | 3.52 | 1.93 | 0.80 | 393 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 4.19 | 1.40 | â | 504 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.