UBC 258
0.66
UTI
0.47
CN
0.94
Cdens
1.0
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
4.2 [arcmin]
- CN 0.47 Poorly populated
- Cdens 0.94 Very dense
- CC3 1.0 Very high quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 258 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (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.
Relatively close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 159.001 | -57.628 | 0.387 | -7.232 | 3.656 | â |
| Almeida et al. | 2025 | 158.88 | -57.604 | â | â | â | â |
| Hunt & Reffert | 2024 | 159.055 | -57.626 | 0.386 | -7.228 | 3.683 | â |
| Cavallo et al. | 2024 | 159.011 | -57.623 | 0.387 | â | â | â |
| Hunt & Reffert | 2023 | 159.055 | -57.626 | 0.386 | -7.228 | 3.683 | â |
| Dias et al. | 2021 | 158.88 | -57.604 | 0.383 | -7.229 | 3.573 | â |
| Cantat-Gaudin et al. | 2020 | 158.917 | -57.615 | 0.393 | -7.237 | 3.609 | â |
| Castro-Ginard et al. | 2020 | 158.88 | -57.609 | 0.39 | -7.227 | 3.591 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.41 | 0.82 | â | 25 | â | 819 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 377* | â | â |
| Cavallo et al. | 2024 | 2.45 | 1.10 | â | 32 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 2.36 | 0.71 | 1.07 | 31 | â | â | â | â |
| Dias et al. | 2021 | 2.41 | 0.82 | â | 25 | 0.197 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.42 | 0.55 | â | 41 | 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: intermediate fit.
Cavallo et al. (2024)
Gold sample.