CWNU 252
0.58
UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
6.0 [N/pc2]
- CN 0.47 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 252 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively 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 absorption, age, and metallicity parameters (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 185.366 | -61.064 | 0.78 | -7.068 | -0.671 | -20.393 |
| Hu & Soubiran | 2025 | 185.484 | -61.05 | â | â | â | â |
| Hunt & Reffert | 2024 | 185.398 | -61.072 | 0.777 | -7.055 | -0.658 | -16.109 |
| Cavallo et al. | 2024 | 185.484 | -61.05 | 0.779 | â | â | â |
| Hunt & Reffert | 2023 | 185.398 | -61.072 | 0.777 | -7.055 | -0.658 | -16.109 |
| He et al. | 2022 | 185.376 | -61.085 | 0.76 | -7.05 | -0.72 | -3.4 |
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 | 1.425 | 0.57 | 0.83 | 212 | 0.270 | 123 | â | â |
| Liu et al. | 2025 | 1.65 | 0.27 | â | 162 | â | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.250(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 123(1) | â | â |
| Cavallo et al. | 2024 | 1.19 | 0.42 | â | 501 | 0.270 | â | â | â |
| Hunt & Reffert | 2023 | 1.23 | 0.72 | 0.83 | 261 | â | â | â | â |
| He et al. | 2022 | 1.62 | 1.14 | â | 100 | 0.805 | 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) 64 along with Harvard_5.
Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P203, along with Harvard_5.
Cavallo et al. (2024)
Gold sample.