CWNU 1718
0.16
UTI
0.25
CN
0.27
Cdens
0.12
CC3
0.3
Clit
0.64
Cdup
Stellar density (N50/rad)
1.4 [N/pc2]
- CN 0.25 Poorly populated
- Cdens 0.27 Loose
- CC3 0.12 Very low quality
- Clit 0.3 Poorly studied
- Cdup 0.64 Likely unique
Overview
CWNU 1718 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate 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 and metallicity parameters (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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 84.808 | 32.599 | 0.482 | -0.257 | -1.4 | â |
| Zhang et al. | 2024 | 84.805 | 32.609 | â | â | â | â |
| Hunt & Reffert | 2024 | 84.805 | 32.609 | 0.478 | -0.27 | -1.392 | â |
| Cavallo et al. | 2024 | 84.827 | 32.542 | 0.475 | â | â | â |
| Hunt & Reffert | 2023 | 84.805 | 32.609 | 0.478 | -0.27 | -1.392 | â |
| He et al. | 2023 | 84.839 | 32.555 | 0.484 | -0.28 | -1.4 | 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 | 2.27 | 1.7 | 1.88 | 85 | 0.150 | 220 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.099(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 220(1) | â | â |
| Cavallo et al. | 2024 | 2.27 | 1.70 | â | 85 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 1.98 | 1.56 | 1.88 | 177 | â | â | â | â |
| He et al. | 2023 | 2.29 | 1.70 | â | 11 | â | 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.