UPK 381
0.56
UTI
0.25
CN
0.44
Cdens
0.62
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
2.2 [N/pc2]
- CN 0.25 Poorly populated
- Cdens 0.44 Loose
- CC3 0.62 Intermediate quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 381 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 (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 95.417 | 29.205 | 1.393 | 0.434 | -2.953 | 4.718 |
| Li et al. | 2025 | 95.506 | 29.107 | 1.378 | 0.437 | -2.987 | â |
| Almeida et al. | 2025 | 95.448 | 29.18 | â | â | â | â |
| Alfonso et al. | 2024 | 95.351 | 29.18 | 1.346 | 0.434 | -2.947 | â |
| Zhang et al. | 2024 | 95.27 | 29.517 | â | â | â | â |
| Cavallo et al. | 2024 | 95.173 | 29.539 | 1.386 | â | â | â |
| Hunt & Reffert | 2023 | 95.27 | 29.517 | 1.382 | 0.384 | -2.936 | 2.477 |
| Almeida et al. | 2023 | 95.438 | 29.135 | â | â | â | â |
| He et al. | 2022 | 95.248 | 29.528 | 1.4 | 0.423 | -2.969 | â |
| Tarricq et al. | 2022 | 95.781 | 29.271 | 1.385 | 0.445 | -2.958 | â |
| Dias et al. | 2021 | 95.448 | 29.18 | 1.346 | 0.437 | -2.997 | 5.646 |
| Cantat-Gaudin et al. | 2020 | 95.506 | 29.107 | 1.378 | 0.437 | -2.987 | â |
| Cantat-Gaudin & Anders | 2020 | 95.5 | 29.205 | 1.377 | 0.48 | -2.986 | â |
| Sim et al. | 2019 | 95.506 | 29.163 | â | 0.48 | -2.96 | 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 | 0.7 | 0.39 | 1.24 | 295 | 0.041 | 128 | 0.58 | â |
| Li et al. | 2025 | 0.66 | 0.39 | â | 318 | -0.050 | â | â | â |
| Almeida et al. | 2025 | 0.70 | 0.39 | â | 366 | â | 112 | â | â |
| Alfonso et al. | 2024 | 0.71 | 0.23 | â | 380 | 0.100 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.148(1) | â | â | â |
| Cavallo et al. | 2024 | 0.70 | 0.62 | â | 234 | 0.080 | â | â | â |
| Hunt & Reffert | 2023 | 0.68 | 0.30 | 1.24 | 201 | â | â | â | â |
| Almeida et al. | 2023 | 0.69 | 0.31 | â | 402 | 0.002 | 143(1) | 0.58 | â |
| He et al. | 2022 | â | 0.70 | â | 200 | â | â | â | â |
| Tarricq et al. | 2022 | 0.70 | â | â | 295 | â | â | â | â |
| Dias et al. | 2021 | 0.70 | 0.39 | â | 366 | 0.100 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.71 | 0.23 | â | 288 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.71 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.71 | â | â | 100 | â | 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: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.