CWNU 361
0.48
UTI
0.28
CN
0.95
Cdens
0.38
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
4.7 [N/pc2]
- CN 0.28 Poorly populated
- Cdens 0.95 Very dense
- CC3 0.38 Low quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 361 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a close distance, below 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 absorption and metallicity parameters (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 | 64.336 | 42.82 | 1.017 | 2.116 | -1.368 | -26.128 |
| Liu et al. | 2025 | 64.35 | 42.81 | 1.02 | 2.09 | -1.37 | -27.1 |
| Zhang et al. | 2024 | 64.354 | 42.809 | â | â | â | â |
| Hunt & Reffert | 2024 | 64.354 | 42.809 | 1.024 | 2.09 | -1.369 | -27.104 |
| Cavallo et al. | 2024 | 64.332 | 42.828 | 1.019 | â | â | â |
| Hunt & Reffert | 2023 | 64.354 | 42.809 | 1.024 | 2.09 | -1.369 | -27.104 |
| He et al. | 2022 | 64.367 | 42.794 | 1.022 | 2.095 | -1.36 | â |
| He et al. | 2022 | 64.354 | 42.804 | 0.98 | 2.12 | -1.37 | 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 | 1.025 | 1.92 | 0.89 | 34 | -0.020 | 115 | â | â |
| Liu et al. | 2025 | 1.54 | 0.49 | â | 107 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.020(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 115(1) | â | â |
| Cavallo et al. | 2024 | 1.07 | 1.92 | â | 34 | 0.100 | â | â | â |
| Hunt & Reffert | 2023 | 0.95 | 1.60 | 0.89 | 125 | â | â | â | â |
| He et al. | 2022 | â | 2.10 | â | 32 | â | â | â | â |
| He et al. | 2022 | 0.98 | 2.10 | â | 32 | -0.930 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 70 along with NGC_1582, and of multiple system 24 along with Gulliver_11, NGC_1582 and HSC_1256.
Palma et al. (2025)
Part of multiple system G92, along with Gulliver_11, NGC_1582 and HSC_1256.
Cavallo et al. (2024)
Gold sample.