CWNU 356
0.57
UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
10.6 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 356 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption 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 | 215.066 | -61.074 | 0.572 | -3.704 | -2.898 | 6.882 |
| Hunt & Reffert | 2024 | 215.058 | -61.081 | 0.584 | -3.673 | -2.888 | 6.953 |
| Cavallo et al. | 2024 | 215.094 | -61.057 | 0.585 | â | â | â |
| Hunt & Reffert | 2023 | 215.058 | -61.081 | 0.584 | -3.673 | -2.888 | 6.953 |
| He et al. | 2022 | 215.061 | -61.073 | 0.57 | -3.71 | -2.9 | 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 | 1.905 | 1.35 | 1.2 | 8 | 0.325 | 302 | â | â |
| Liu et al. | 2025 | 2.94 | 0.53 | â | 9 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 302(1) | â | â |
| Cavallo et al. | 2024 | 1.62 | 1.21 | â | 17 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 1.60 | 1.49 | 1.20 | 6 | â | â | â | â |
| He et al. | 2022 | 2.19 | 1.80 | â | 5 | 0.680 | 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) 69 along with Theia_2166.
Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P205, along with Loden_1256.
Cavallo et al. (2024)
Silver sample.