CWNU 1062
0.28
UTI
0.0
CN
0.16
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
0.8 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.16 Very loose
- CC3 0.75 High quality
- Clit 0.25 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 1062 is a sparse, very loose object of high C3 quality. Its parallax locates it at a very 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 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 | 173.668 | 16.849 | 3.227 | -9.106 | -1.586 | 12.3 |
| Zhang et al. | 2024 | 173.701 | 16.845 | â | â | â | â |
| Cavallo et al. | 2024 | 173.425 | 16.927 | 3.212 | â | â | â |
| Hunt & Reffert | 2023 | 173.701 | 16.845 | 3.202 | -9.193 | -1.582 | 8.144 |
| He et al. | 2022 | 173.576 | 17.029 | 3.208 | -9.11 | -1.583 | 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 | 0.31 | 0.49 | 0.39 | 24 | 0.015 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.010(1) | â | â | â |
| Cavallo et al. | 2024 | 0.32 | 0.49 | â | 24 | 0.040 | â | â | â |
| Hunt & Reffert | 2023 | 0.30 | 0.06 | 0.39 | 24 | â | â | â | â |
| He et al. | 2022 | â | 0.50 | â | 28 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.