CWNU 512
0.19
UTI
0.0
CN
0.1
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
24.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.1 Very loose
- CC3 0.38 Low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 512 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
Moderate extinction
Metal-poor
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 5.086 | 68.902 | 1.05 | -2.847 | -0.142 | -21.482 |
| Hunt & Reffert | 2024 | 5.095 | 68.734 | 1.046 | -2.845 | -0.155 | -23.788 |
| Cavallo et al. | 2024 | 4.603 | 68.921 | 1.044 | â | â | â |
| Hunt & Reffert | 2023 | 5.095 | 68.734 | 1.046 | -2.845 | -0.155 | -23.788 |
| He et al. | 2022 | 6.213 | 68.937 | 1.05 | -2.8 | -0.01 | 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 | 70* | â | â |
| Cavallo et al. | 2024 | 1.11 | 3.03 | â | 35 | 0.210 | â | â | â |
| Hunt & Reffert | 2023 | 0.90 | 2.93 | 1.84 | 93 | â | â | â | â |
| He et al. | 2022 | 1.51 | 2.64 | â | 3 | -2.028 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.