CWNU 1024
0.56
UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
56.6 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
CWNU 1024 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
Very close
Low 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 | 104.396 | -26.866 | 2.514 | -6.018 | 6.017 | 21.44 |
| Cavallo et al. | 2024 | 103.156 | -25.587 | 2.497 | â | â | â |
| Hunt & Reffert | 2023 | 104.286 | -27.392 | 2.495 | -5.545 | 6.018 | 21.594 |
| He et al. | 2022 | 104.451 | -26.85 | 2.521 | -6.046 | 6.01 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.41 | 0.43 | â | 11 | -0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.39 | 0.17 | 0.73 | 32 | â | â | â | â |
| He et al. | 2022 | â | 0.35 | â | 40 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.