CWNU 2592
0.36
UTI
0.3
CN
0.23
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
1.1 [N/pc2]
- CN 0.3 Poorly populated
- Cdens 0.23 Very loose
- 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 2592 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate 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 | 297.783 | 22.746 | 0.239 | -2.482 | -4.937 | -15.334 |
| Hunt & Reffert | 2024 | 297.688 | 22.659 | 0.225 | -2.509 | -4.908 | â |
| Cavallo et al. | 2024 | 297.75 | 22.723 | 0.232 | â | â | â |
| Hunt & Reffert | 2023 | 297.688 | 22.659 | 0.225 | -2.509 | -4.908 | â |
| He et al. | 2023 | 297.807 | 22.791 | 0.244 | -2.486 | -4.933 | 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 | 4.09 | 2.59 | 1.49 | 27 | 0.390 | 210 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 210(1) | â | â |
| Cavallo et al. | 2024 | 4.09 | 2.56 | â | 28 | 0.390 | â | â | â |
| Hunt & Reffert | 2023 | 3.81 | 2.59 | 1.49 | 27 | â | â | â | â |
| He et al. | 2023 | 4.27 | 2.85 | â | 9 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Silver sample.