CWNU 1190
0.51
UTI
0.31
CN
1.0
Cdens
0.62
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
6.2 [N/pc2]
- CN 0.31 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.3 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 1190 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (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 | 69.347 | 45.348 | 0.844 | -0.421 | -1.655 | 3.458 |
| Zhang et al. | 2024 | 69.342 | 45.395 | â | â | â | â |
| Hunt & Reffert | 2024 | 69.342 | 45.395 | 0.837 | -0.474 | -1.63 | 24.069 |
| Cavallo et al. | 2024 | 69.286 | 45.372 | 0.834 | â | â | â |
| Hunt & Reffert | 2023 | 69.342 | 45.395 | 0.837 | -0.474 | -1.63 | 24.069 |
| He et al. | 2022 | 69.257 | 45.342 | 0.868 | -0.445 | -1.735 | 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 | 1.27 | 1.04 | 0.8 | 5 | 0.115 | 95 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.009(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 95(1) | â | â |
| Cavallo et al. | 2024 | 1.40 | 1.04 | â | 5 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 1.14 | 1.21 | 0.80 | 6 | â | â | â | â |
| He et al. | 2022 | â | 0.85 | â | 5 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Silver sample.