CWNU 406
0.44
UTI
0.28
CN
0.38
Cdens
0.75
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
1.9 [N/pc2]
- CN 0.28 Poorly populated
- Cdens 0.38 Loose
- CC3 0.75 High quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 406 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 absorption, age, and metallicity parameters (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 | 91.272 | 20.84 | 0.982 | 1.568 | -2.266 | -1.082 |
| Liu et al. | 2025 | 91.4 | 20.81 | 0.98 | 1.61 | -2.28 | -4.57 |
| Zhang et al. | 2024 | 91.399 | 20.814 | â | â | â | â |
| Hunt & Reffert | 2024 | 91.399 | 20.814 | 0.98 | 1.612 | -2.281 | -4.574 |
| Cavallo et al. | 2024 | 91.241 | 20.948 | 0.976 | â | â | â |
| Hunt & Reffert | 2023 | 91.399 | 20.814 | 0.98 | 1.612 | -2.281 | -4.574 |
| He et al. | 2022 | 91.265 | 20.817 | 0.982 | 1.555 | -2.232 | â |
| He et al. | 2022 | 91.319 | 20.841 | 0.98 | 1.59 | -2.25 | 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 | 1.045 | 0.66 | 0.75 | 181 | -0.076 | 149 | â | â |
| Liu et al. | 2025 | 1.51 | 0.28 | â | 219 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.076(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 149(1) | â | â |
| Cavallo et al. | 2024 | 0.99 | 0.62 | â | 479 | 0.110 | â | â | â |
| Hunt & Reffert | 2023 | 0.96 | 0.66 | 0.75 | 181 | â | â | â | â |
| He et al. | 2022 | â | 0.85 | â | 79 | â | â | â | â |
| He et al. | 2022 | 1.10 | 1.20 | â | 63 | -0.642 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 44 along with COIN-Gaia_24, and as tidal capture (resonant trapping binary) 71 along with HSC_1507, and of multiple system 19 along with COIN-Gaia_24 and HSC_1507.
Palma et al. (2025)
Part of multiple system G64, along with COIN-Gaia_24 and HSC_1507.
Cavallo et al. (2024)
Gold sample.