CWNU 525
0.44
UTI
0.43
CN
0.23
Cdens
0.75
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
1.2 [N/pc2]
- CN 0.43 Poorly populated
- Cdens 0.23 Very loose
- CC3 0.75 High quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
CWNU 525 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low 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 | 84.825 | 37.513 | 0.86 | -0.335 | -2.8 | 2.503 |
| Zhang et al. | 2024 | 84.926 | 37.501 | â | â | â | â |
| Hunt & Reffert | 2024 | 84.926 | 37.501 | 0.853 | -0.325 | -2.797 | 2.583 |
| Cavallo et al. | 2024 | 84.763 | 37.518 | 0.856 | â | â | â |
| Hunt & Reffert | 2023 | 84.926 | 37.501 | 0.853 | -0.325 | -2.797 | 2.583 |
| He et al. | 2022 | 359.297 | 55.809 | 2.515 | 8.227 | -3.68 | â |
| He et al. | 2022 | 84.805 | 37.492 | 0.87 | -0.36 | -2.79 | 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 | 1.14 | 0.74 | 1.1 | 20 | -0.280 | 262 | â | â |
| Liu et al. | 2025 | 1.72 | 0.32 | â | 21 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.112(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 262(1) | â | â |
| Cavallo et al. | 2024 | 1.17 | 1.05 | â | 9 | -0.280 | â | â | â |
| Hunt & Reffert | 2023 | 1.11 | 0.74 | 1.10 | 28 | â | â | â | â |
| He et al. | 2022 | â | 0.20 | â | 13 | â | â | â | â |
| He et al. | 2022 | 0.89 | 0.96 | â | 20 | -0.930 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Liu et al. (2025)
Classified as primordial binary cluster 81 along with HSC_1350.
Palma et al. (2025)
Part of multiple system G113, along with HSC_1350, NGC_1912 and Teutsch_89.
Cavallo et al. (2024)
Gold sample.