CWNU 105
0.34
UTI
0.0
CN
0.56
Cdens
0.38
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
5.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.56 Moderately dense
- CC3 0.38 Low quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 105 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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 | 58.99 | 38.464 | 0.528 | 0.195 | 0.034 | -35.758 |
| Hu & Soubiran | 2025 | 58.992 | 38.474 | â | â | â | â |
| Zhang et al. | 2024 | 58.957 | 38.466 | â | â | â | â |
| Hunt & Reffert | 2024 | 58.957 | 38.466 | 0.535 | 0.197 | 0.056 | -35.36 |
| Cavallo et al. | 2024 | 58.992 | 38.474 | 0.529 | â | â | â |
| Hunt & Reffert | 2023 | 58.957 | 38.466 | 0.535 | 0.197 | 0.056 | -35.36 |
| He et al. | 2022 | 58.996 | 38.5 | 0.52 | 0.19 | 0.03 | -35.4 |
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 | 1.77 | 2.26 | 1.99 | 631 | 0.091 | 134 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | 0.030(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.153(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 134(1) | â | â |
| Cavallo et al. | 2024 | 1.62 | 2.54 | â | 1122 | -0.210 | â | â | â |
| Hunt & Reffert | 2023 | 1.77 | 2.26 | 1.99 | 605 | â | â | â | â |
| He et al. | 2022 | 1.95 | 2.22 | â | 631 | 0.862 | â | â | â |
(N): Indicates that are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Gold sample.