CWNU 10
0.07
UTI
0.26
CN
0.55
Cdens
0.38
CC3
0.3
Clit
0.19
Cdup
Stellar density (N50/rad)
2.7 [N/pc2]
- CN 0.26 Poorly populated
- Cdens 0.55 Moderately dense
- CC3 0.38 Low quality
- Clit 0.3 Poorly studied
- Cdup 0.19 Likely duplicate
Overview
CWNU 10 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a 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 metallicity parameter (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously 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 | 95.286 | 18.841 | 1.011 | -1.801 | -2.851 | -10.86 |
| Zhang et al. | 2024 | 95.318 | 18.827 | â | â | â | â |
| Hunt & Reffert | 2024 | 95.318 | 18.827 | 0.989 | -1.763 | -2.849 | 0.035 |
| Cavallo et al. | 2024 | 95.254 | 18.896 | 0.987 | â | â | â |
| Hunt & Reffert | 2023 | 95.318 | 18.827 | 0.989 | -1.763 | -2.849 | 0.035 |
| He et al. | 2022 | 95.281 | 18.871 | 1.01 | -1.74 | -2.85 | 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 | 1.07 | 0.79 | 1.69 | 251 | 0.250 | 131 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.237(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 131(1) | â | â |
| Cavallo et al. | 2024 | 1.07 | 0.88 | â | 186 | 0.250 | â | â | â |
| Hunt & Reffert | 2023 | 0.95 | 0.79 | 1.69 | 286 | â | â | â | â |
| He et al. | 2022 | 1.17 | 0.78 | â | 251 | 0.968 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.