UBC 248
0.66
UTI
0.61
CN
1.0
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
5.4 [N/pc2]
- CN 0.61 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 248 is a moderately populated, very dense object of very high 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 137.98 | -52.233 | 0.327 | -4.084 | 3.925 | 23.664 |
| Almeida et al. | 2025 | 137.985 | -52.244 | â | â | â | â |
| Hunt & Reffert | 2024 | 137.978 | -52.23 | 0.328 | -4.072 | 3.925 | 19.254 |
| Cavallo et al. | 2024 | 137.955 | -52.227 | 0.33 | â | â | â |
| Hunt & Reffert | 2023 | 137.978 | -52.23 | 0.328 | -4.072 | 3.925 | 19.254 |
| Dias et al. | 2021 | 137.985 | -52.244 | 0.28 | -4.098 | 3.892 | 24.152 |
| Castro-Ginard et al. | 2020 | 137.986 | -52.235 | 0.3 | -4.108 | 3.907 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.61 | 1.51 | 0.71 | 194 | -0.298 | 551 | â | â |
| Almeida et al. | 2025 | 2.61 | 1.51 | â | 187 | â | 649 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 453(1) | â | â |
| Cavallo et al. | 2024 | 2.23 | 1.66 | â | 355 | -0.670 | â | â | â |
| Hunt & Reffert | 2023 | 2.73 | 1.34 | 0.71 | 201 | â | â | â | â |
| Dias et al. | 2021 | 2.61 | 1.51 | â | 187 | 0.074 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Castro-Ginard et al. (2020)
Coincidence with Sim et al. (2019, J. Korean Astron. Soc., 52, 145) or Liu & Pang (2019ApJS..245...32L), see Sect. 4.1.5.