CWNU 1076
(OCSN 173)
0.52
UTI
0.46
CN
0.68
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
3.4 [N/pc2]
- CN 0.46 Poorly populated
- Cdens 0.68 Moderately dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1076 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a very close distance, near 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 40.719 | 56.755 | 2.789 | 8.776 | -4.026 | -1.586 |
| Wei et al. | 2025 | 40.361 | 56.864 | 2.788 | 8.74 | -4.005 | â |
| Zhang et al. | 2024 | 41.235 | 56.709 | â | â | â | â |
| Cavallo et al. | 2024 | 40.756 | 56.882 | 2.794 | â | â | â |
| Hunt & Reffert | 2023 | 41.235 | 56.709 | 2.772 | 8.698 | -4.095 | -2.327 |
| Qin et al. | 2023 | 40.93 | 56.68 | 2.8 | 8.71 | -3.98 | -3.17 |
| He et al. | 2022 | 40.98 | 56.579 | 2.77 | 8.78 | -4.026 | 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 | 0.37 | 0.51 | 0.56 | 111 | 0.250 | 78 | 0.31 | â |
| Wei et al. | 2025 | 0.38 | 0.51 | â | 135 | 0.250 | 78 | 0.31 | â |
| Zhang et al. | 2024 | â | â | â | â | -0.049(1) | â | â | â |
| Cavallo et al. | 2024 | 0.36 | 0.64 | â | 145 | 0.310 | â | â | â |
| Hunt & Reffert | 2023 | 0.34 | 0.36 | 0.56 | 111 | â | â | â | â |
| Qin et al. | 2023 | 0.40 | 0.53 | â | 100 | â | â | â | â |
| He et al. | 2022 | â | 0.45 | â | 79 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P291, along with Stock_2.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.