UPK 379
0.51
UTI
0.28
CN
0.29
Cdens
0.5
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
19.6 [arcmin]
- CN 0.28 Poorly populated
- Cdens 0.29 Loose
- CC3 0.5 Intermediate quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 379 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, above 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 age and metallicity parameters (see Parameters). It is well-studied in the literature.
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 | 94.211 | 30.783 | 1.301 | -1.017 | -4.33 | 8.336 |
| Almeida et al. | 2025 | 93.887 | 30.814 | â | â | â | â |
| Alfonso et al. | 2024 | 94.195 | 30.905 | 1.271 | -0.975 | -4.297 | â |
| Zhang et al. | 2024 | 94.219 | 30.744 | â | â | â | â |
| Hunt & Reffert | 2024 | 94.219 | 30.744 | 1.302 | -0.983 | -4.314 | 7.446 |
| Cavallo et al. | 2024 | 94.206 | 30.791 | 1.302 | â | â | â |
| Hunt & Reffert | 2023 | 94.219 | 30.744 | 1.302 | -0.983 | -4.314 | 7.446 |
| Almeida et al. | 2023 | 93.785 | 30.829 | â | â | â | â |
| He et al. | 2022 | 94.199 | 30.689 | 1.303 | -1.062 | -4.367 | â |
| Tarricq et al. | 2022 | 94.172 | 30.907 | 1.328 | -1.037 | -4.332 | â |
| Dias et al. | 2021 | 93.887 | 30.814 | 1.299 | -0.933 | -4.311 | â |
| Cantat-Gaudin et al. | 2020 | 94.071 | 30.794 | 1.284 | -0.968 | -4.325 | â |
| Cantat-Gaudin & Anders | 2020 | 94.071 | 30.794 | 1.279 | -0.959 | -4.327 | â |
| Sim et al. | 2019 | 94.131 | 30.894 | â | -0.97 | -4.29 | 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 | 0.73 | 0.94 | â | 419 | â | 117 | â | â |
| Alfonso et al. | 2024 | 0.77 | 0.69 | â | 1054 | -0.153 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.222* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 78* | â | â |
| Cavallo et al. | 2024 | 0.77 | 1.33 | â | 302 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 0.73 | 0.78 | 1.67 | 466 | â | â | â | â |
| Almeida et al. | 2023 | 0.74 | 0.79 | â | 139 | 0.009 | 176* | 0.53 | â |
| He et al. | 2022 | â | 1.45 | â | 224 | â | â | â | â |
| Tarricq et al. | 2022 | 0.76 | â | â | 490 | â | â | â | â |
| Dias et al. | 2021 | 0.73 | 0.94 | â | 419 | -0.153 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.77 | 0.69 | â | 457 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.76 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.77 | â | â | 631 | 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.