UBC 379
0.64
UTI
0.56
CN
1.0
Cdens
0.75
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
5.3 [N/pc2]
- CN 0.56 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 379 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 313.269 | 48.548 | 0.371 | -2.537 | -2.431 | â |
| Almeida et al. | 2025 | 313.269 | 48.534 | â | â | â | â |
| Hunt & Reffert | 2024 | 313.251 | 48.571 | 0.357 | -2.528 | -2.464 | â |
| Celli et al. | 2024 | 313.264 | 48.538 | â | â | â | â |
| Cavallo et al. | 2024 | 313.284 | 48.535 | 0.37 | â | â | â |
| Hunt & Reffert | 2023 | 313.251 | 48.571 | 0.357 | -2.528 | -2.464 | â |
| Dias et al. | 2021 | 313.269 | 48.534 | 0.368 | -2.534 | -2.452 | â |
| Cantat-Gaudin et al. | 2020 | 313.264 | 48.538 | 0.364 | -2.531 | -2.442 | â |
| Castro-Ginard et al. | 2020 | 313.256 | 48.542 | 0.365 | -2.527 | -2.466 | 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 | 2.46 | 2.66 | 1.27 | 22 | 0.492 | 420 | â | â |
| Almeida et al. | 2025 | 2.46 | 2.66 | â | 22 | â | 420 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 295(1) | â | â |
| Celli et al. | 2024 | â | â | â | 18 | â | 431 | â | â |
| Cavallo et al. | 2024 | 2.52 | 2.92 | â | 69 | 0.540 | â | â | â |
| Hunt & Reffert | 2023 | 2.46 | 2.83 | 1.27 | 97 | â | â | â | â |
| Dias et al. | 2021 | 2.46 | 2.66 | â | 22 | 0.445 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.57 | 2.56 | â | 18 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair (not dynamically associated) P110, along with CWNU_2338.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.