CWWDL 14129
0.06
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members)
12.5 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.12 Likely duplicate
Overview
CWWDL 14129 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, very young cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Close
Moderate extinction
Metal-poor
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 229.625 | -60.979 | 1.187 | -3.134 | -4.106 | -7.878 |
| Wei et al. | 2025 | 229.775 | -60.926 | 1.192 | -3.045 | -4.093 | â |
| Chi et al. | 2023 | 229.741 | -60.986 | 1.191 | -3.098 | -4.073 | -9.878 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Wei et al. | 2025 | 0.75 | 1.02 | â | 15 | -0.750 | 635 | 0.60 | â |
| Chi et al. | 2023 | â | â | â | 0 | -0.880 | â | â | â |
