CWNU 1126
0.39
UTI
0.36
CN
0.82
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
4.1 [N/pc2]
- CN 0.36 Poorly populated
- Cdens 0.82 Dense
- CC3 0.75 High quality
- Clit 0.0 Rarely 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 1126 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with a later 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 | 332.1 | 64.071 | 1.082 | -1.462 | -3.226 | -21.606 |
| Liu et al. | 2025 | 332.32 | 64.08 | 1.08 | -1.41 | -3.25 | -25.15 |
| Hunt & Reffert | 2024 | 332.32 | 64.076 | 1.075 | -1.414 | -3.246 | -25.15 |
| Cavallo et al. | 2024 | 332.186 | 64.095 | 1.073 | â | â | â |
| Hunt & Reffert | 2023 | 332.32 | 64.076 | 1.075 | -1.414 | -3.246 | -25.15 |
| He et al. | 2022 | 332.254 | 64.073 | 1.077 | -1.452 | -3.22 | 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 | 1.03 | 0.98 | 1.4 | 12 | 0.150 | 126 | â | â |
| Liu et al. | 2025 | 1.14 | 0.37 | â | 23 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 126(1) | â | â |
| Cavallo et al. | 2024 | 1.03 | 1.30 | â | 8 | 0.150 | â | â | â |
| Hunt & Reffert | 2023 | 0.90 | 1.06 | 1.40 | 16 | â | â | â | â |
| He et al. | 2022 | â | 0.90 | â | 8 | â | 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 95 along with OC_0185, and of multiple system 34 along with Pismis-Moreno_1, CWNU_1228, HSC_853, OC_0185 and HSC_824.
Palma et al. (2025)
Part of multiple system G30, along with Pismis-Moreno_1, OC_0185, HSC_824, CWNU_1228, FSR_0398 and CWNU_446.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.98 (50th percentile).