CWNU 2592
0.36
UTI
0.3
CN
0.23
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
4.2 [arcmin]
- CN 0.3 Poorly populated
- Cdens 0.23 Very loose
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
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.
Distant
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 210* | 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 |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.