CWNU 2792
0.51
UTI
0.34
CN
0.98
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
4.9 [N/pc2]
- CN 0.34 Poorly populated
- Cdens 0.98 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 2792 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 | 225.08 | -58.379 | 0.408 | -4.474 | -2.806 | -26.829 |
| Hunt & Reffert | 2024 | 225.091 | -58.36 | 0.412 | -4.468 | -2.794 | -38.806 |
| Cavallo et al. | 2024 | 225.058 | -58.368 | 0.409 | â | â | â |
| Hunt & Reffert | 2023 | 225.091 | -58.36 | 0.412 | -4.468 | -2.794 | -38.806 |
| He et al. | 2023 | 225.039 | -58.411 | 0.405 | -4.516 | -2.812 | -26.4 |
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 | 2.24 | 4.29 | 2.41 | 219 | 0.240 | 651 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 651(1) | â | â |
| Cavallo et al. | 2024 | 1.97 | 4.02 | â | 219 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 2.26 | 4.29 | 2.41 | 100 | â | â | â | â |
| He et al. | 2023 | 2.24 | 4.50 | â | 224 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Palma et al. (2025)
Part of multiple system G39, along with HSC_2678, CWNU_1560 and CWNU_1528.
Cavallo et al. (2024)
Gold sample.