UBC 175
0.80
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
12.1 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UBC 175 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low 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 well-studied in the literature.
Relatively close
Low 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 | 344.432 | 54.385 | 0.739 | 1.451 | -0.789 | -30.0 |
| Li et al. | 2025 | 344.451 | 54.401 | 0.721 | 1.432 | -0.726 | â |
| Hu & Soubiran | 2025 | 344.476 | 54.354 | â | â | â | â |
| Wei et al. | 2025 | 344.354 | 54.383 | 0.743 | 1.475 | -0.744 | â |
| Almeida et al. | 2025 | 344.43 | 54.378 | â | â | â | â |
| Zhang et al. | 2024 | 344.489 | 54.434 | â | â | â | â |
| Hunt & Reffert | 2024 | 344.489 | 54.434 | 0.738 | 1.466 | -0.801 | -29.312 |
| Cavallo et al. | 2024 | 344.476 | 54.354 | 0.737 | â | â | â |
| Hunt & Reffert | 2023 | 344.489 | 54.434 | 0.738 | 1.466 | -0.801 | -29.312 |
| Almeida et al. | 2023 | 344.432 | 54.375 | â | â | â | â |
| Tarricq et al. | 2022 | 344.443 | 54.42 | 0.735 | 1.46 | -0.793 | â |
| Dias et al. | 2021 | 344.43 | 54.378 | 0.728 | 1.418 | -0.725 | â |
| Cantat-Gaudin et al. | 2020 | 344.451 | 54.401 | 0.721 | 1.432 | -0.726 | â |
| Castro-Ginard et al. | 2020 | 344.448 | 54.387 | 0.722 | 1.435 | -0.726 | 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 | 1.22 | 0.66 | â | 738 | 0.061 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.030* | â | â | â |
| Wei et al. | 2025 | 1.69 | 0.91 | â | 576 | 0.250 | 688 | 0.80 | â |
| Almeida et al. | 2025 | 1.32 | 1.07 | â | 445 | â | 245 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.017* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 359* | â | â |
| Cavallo et al. | 2024 | 1.39 | 0.81 | â | 537 | 0.490 | â | â | â |
| Hunt & Reffert | 2023 | 1.29 | 0.80 | 0.53 | 359 | â | â | â | â |
| Almeida et al. | 2023 | 1.27 | 1.08 | â | 452 | -0.016 | 299* | 0.59 | â |
| Tarricq et al. | 2022 | 1.30 | â | â | 513 | â | â | â | â |
| Dias et al. | 2021 | 1.32 | 1.07 | â | 445 | 0.195 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.34 | 0.88 | â | 468 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.