CWNU 1458
0.44
UTI
0.32
CN
0.64
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
3.2 [N/pc2]
- CN 0.32 Poorly populated
- Cdens 0.64 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 1458 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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 | 124.992 | -44.509 | 0.581 | -5.232 | 5.016 | â |
| Hunt & Reffert | 2024 | 124.976 | -44.479 | 0.568 | -5.234 | 5.012 | â |
| Cavallo et al. | 2024 | 125.048 | -44.57 | 0.575 | â | â | â |
| Hunt & Reffert | 2023 | 124.976 | -44.479 | 0.568 | -5.234 | 5.012 | â |
| He et al. | 2023 | 124.998 | -44.531 | 0.584 | -5.232 | 5.016 | 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 | 1.66 | 0.95 | 0.54 | 55 | 0.070 | 94 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 94(1) | â | â |
| Cavallo et al. | 2024 | 1.75 | 1.17 | â | 55 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 1.66 | 0.74 | 0.54 | 99 | â | â | â | â |
| He et al. | 2023 | 1.62 | 0.95 | â | 35 | 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.