CWNU 350
0.28
UTI
0.0
CN
0.29
Cdens
0.38
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
12.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.29 Loose
- CC3 0.38 Low quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 350 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, above 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 age parameter (see Parameters). It is poorly studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 76.425 | 45.993 | 0.903 | -0.549 | -1.768 | -34.29 |
| Hu & Soubiran | 2025 | 76.476 | 45.943 | â | â | â | â |
| Zhang et al. | 2024 | 76.466 | 45.969 | â | â | â | â |
| Hunt & Reffert | 2024 | 76.466 | 45.969 | 0.904 | -0.504 | -1.757 | -22.79 |
| Cavallo et al. | 2024 | 76.476 | 45.943 | 0.904 | â | â | â |
| Hunt & Reffert | 2023 | 76.466 | 45.969 | 0.904 | -0.504 | -1.757 | -22.79 |
| He et al. | 2022 | 76.361 | 46.033 | 0.94 | -0.55 | -1.74 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.230* | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.126* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 102* | â | â |
| Cavallo et al. | 2024 | 1.06 | 1.09 | â | 1549 | -0.060 | â | â | â |
| Hunt & Reffert | 2023 | 1.05 | 0.70 | 0.90 | 33 | â | â | â | â |
| He et al. | 2022 | 1.05 | 1.02 | â | 79 | 0.370 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.