CWNU 26
0.44
UTI
0.39
CN
0.61
Cdens
0.5
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
3.1 [N/pc2]
- CN 0.39 Poorly populated
- Cdens 0.61 Moderately dense
- CC3 0.5 Intermediate quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 26 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is poorly studied in the literature.
Note: This object shares a moderate 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 | 93.853 | 13.808 | 0.441 | -0.704 | -1.044 | â |
| Zhang et al. | 2024 | 93.868 | 13.785 | â | â | â | â |
| Hunt & Reffert | 2024 | 93.868 | 13.785 | 0.432 | -0.791 | -1.046 | â |
| Cavallo et al. | 2024 | 93.842 | 13.728 | 0.432 | â | â | â |
| Hunt & Reffert | 2023 | 93.868 | 13.785 | 0.432 | -0.791 | -1.046 | â |
| He et al. | 2022 | 93.846 | 13.784 | 0.44 | -0.56 | -1.07 | 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 | 2.1 | 1.25 | 0.35 | 60 | -0.419 | 111 | â | â |
| Liu et al. | 2025 | 3.45 | 0.44 | â | 47 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.183(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 111(1) | â | â |
| Cavallo et al. | 2024 | 1.98 | 1.52 | â | 28 | -0.420 | â | â | â |
| Hunt & Reffert | 2023 | 2.22 | 1.30 | 0.35 | 74 | â | â | â | â |
| He et al. | 2022 | 1.78 | 1.20 | â | 158 | -0.419 | 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) 48 along with Theia_2249.
Palma et al. (2025)
Classified as optical pair P360, along with Theia_2249.
Cavallo et al. (2024)
Gold sample.