CWNU 413
0.52
UTI
0.39
CN
0.94
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
4.7 [N/pc2]
- CN 0.39 Poorly populated
- Cdens 0.94 Very 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 413 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the metallicity 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 | 303.999 | 30.308 | 0.83 | -2.684 | -8.606 | 9.911 |
| Hunt & Reffert | 2024 | 304.016 | 30.332 | 0.841 | -2.698 | -8.578 | 6.201 |
| Cavallo et al. | 2024 | 304.25 | 30.437 | 0.839 | â | â | â |
| Hunt & Reffert | 2023 | 304.016 | 30.332 | 0.841 | -2.698 | -8.578 | 6.201 |
| He et al. | 2022 | 304.012 | 30.324 | 0.83 | -2.66 | -8.6 | 6.1 |
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 | 1.16 | 1.8 | 2.47 | 229 | 0.509 | 95 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 95(1) | â | â |
| Cavallo et al. | 2024 | 1.35 | 2.09 | â | 178 | 0.050 | â | â | â |
| Hunt & Reffert | 2023 | 1.16 | 1.77 | 2.47 | 229 | â | â | â | â |
| He et al. | 2022 | 1.15 | 1.80 | â | 251 | 0.968 | 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.