CWNU 2413
0.44
UTI
0.39
CN
0.43
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
6.4 [arcmin]
- CN 0.39 Poorly populated
- Cdens 0.43 Loose
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 2413 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Relatively close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 160.385 | -56.6 | 0.438 | -7.815 | 3.426 | -10.708 |
| Hu & Soubiran | 2025 | 160.423 | -56.614 | â | â | â | â |
| Hunt & Reffert | 2024 | 160.347 | -56.639 | 0.436 | -7.855 | 3.442 | 7.778 |
| Cavallo et al. | 2024 | 160.423 | -56.614 | 0.435 | â | â | â |
| Hunt & Reffert | 2023 | 160.347 | -56.639 | 0.436 | -7.855 | 3.442 | 7.778 |
| He et al. | 2023 | 160.519 | -56.598 | 0.435 | -7.805 | 3.414 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.120* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 151* | â | â |
| Cavallo et al. | 2024 | 2.11 | 0.80 | â | 513 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 2.09 | 0.86 | 1.20 | 328 | â | â | â | â |
| He et al. | 2023 | 2.14 | 1.05 | â | 447 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.