CWNU 2585
0.31
UTI
0.6
CN
0.42
Cdens
0.75
CC3
0.31
Clit
0.65
Cdup
Radius (P>50% members)
6.7 [arcmin]
- CN 0.6 Moderately populated
- Cdens 0.42 Loose
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 0.65 Likely unique
Overview
CWNU 2585 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.
Relatively close
High extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 358.398 | 68.232 | 0.339 | -2.828 | 0.183 | -53.82 |
| Hu & Soubiran | 2025 | 358.304 | 68.242 | â | â | â | â |
| Hunt & Reffert | 2024 | 358.583 | 68.222 | 0.334 | -2.82 | 0.163 | -52.248 |
| Cavallo et al. | 2024 | 358.304 | 68.242 | 0.337 | â | â | â |
| Hunt & Reffert | 2023 | 358.583 | 68.222 | 0.334 | -2.82 | 0.163 | -52.248 |
| He et al. | 2023 | 358.414 | 68.233 | 0.347 | -2.826 | 0.185 | -52.41 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | 0.000* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 603* | â | â |
| Cavallo et al. | 2024 | 2.63 | 3.68 | â | 1000 | -0.540 | â | â | â |
| Hunt & Reffert | 2023 | 2.73 | 3.23 | 1.42 | 1346 | â | â | â | â |
| He et al. | 2023 | 2.69 | 3.10 | â | 2239 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.