CWNU 1290
0.46
UTI
0.49
CN
0.58
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
2.9 [N/pc2]
- CN 0.49 Poorly populated
- Cdens 0.58 Moderately dense
- 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 1290 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 143.161 | -55.828 | 0.368 | -5.687 | 4.481 | 0.811 |
| Hunt & Reffert | 2024 | 143.155 | -55.824 | 0.353 | -5.703 | 4.502 | â |
| Cavallo et al. | 2024 | 143.175 | -55.829 | 0.356 | â | â | â |
| Hunt & Reffert | 2023 | 143.155 | -55.824 | 0.353 | -5.703 | 4.502 | â |
| He et al. | 2023 | 143.176 | -55.816 | 0.368 | -5.722 | 4.484 | -1.39 |
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 | 2.63 | 3.51 | 2.3 | 331 | -0.110 | 369 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 369(1) | â | â |
| Cavallo et al. | 2024 | 2.63 | 3.51 | â | 331 | -0.110 | â | â | â |
| Hunt & Reffert | 2023 | 2.50 | 2.67 | 2.30 | 514 | â | â | â | â |
| He et al. | 2023 | 2.69 | 3.60 | â | 316 | 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.