CWNU 1459
0.63
UTI
0.56
CN
1.0
Cdens
1.0
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
6.9 [N/pc2]
- CN 0.56 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1459 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It was recently reported 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 | 145.59 | -38.461 | 0.242 | -5.673 | 4.28 | 30.489 |
| Hu & Soubiran | 2025 | 145.6 | -38.463 | â | â | â | â |
| Hunt & Reffert | 2024 | 145.585 | -38.458 | 0.234 | -5.674 | 4.285 | 30.44 |
| Cavallo et al. | 2024 | 145.6 | -38.463 | 0.236 | â | â | â |
| Hunt & Reffert | 2023 | 145.585 | -38.458 | 0.234 | -5.674 | 4.285 | 30.44 |
| He et al. | 2023 | 145.591 | -38.455 | 0.243 | -5.681 | 4.269 | 30.49 |
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 | 3.76 | 0.67 | 0.25 | 2742 | -0.280 | 394 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.190(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 394(1) | â | â |
| Cavallo et al. | 2024 | 2.73 | 0.67 | â | 5012 | -0.370 | â | â | â |
| Hunt & Reffert | 2023 | 3.76 | 0.30 | 0.25 | 2742 | â | â | â | â |
| He et al. | 2023 | 5.13 | 1.90 | â | 316 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.