CWNU 124
0.38
UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
8.9 [N/pc2]
- CN 0.0 Sparse
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 124 is a sparse, very dense object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (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 | 349.188 | 64.718 | 1.001 | 0.626 | -0.457 | -33.512 |
| Hunt & Reffert | 2024 | 349.21 | 64.694 | 1.0 | 0.623 | -0.443 | -20.639 |
| Cavallo et al. | 2024 | 349.177 | 64.671 | 0.999 | â | â | â |
| Hunt & Reffert | 2023 | 349.21 | 64.694 | 1.0 | 0.623 | -0.443 | -20.639 |
| He et al. | 2022 | 349.121 | 64.689 | 1.0 | 0.63 | -0.46 | 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 | 1.04 | 2.1 | 0.48 | 162 | 0.545 | 87 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 87(1) | â | â |
| Cavallo et al. | 2024 | 1.04 | 1.84 | â | 162 | 0.410 | â | â | â |
| Hunt & Reffert | 2023 | 1.03 | 2.10 | 0.48 | 230 | â | â | â | â |
| He et al. | 2022 | 1.20 | 2.22 | â | 158 | 0.680 | 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.