CWWL 3078
0.61
UTI
0.56
CN
0.9
Cdens
1.0
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
4.5 [N/pc2]
- CN 0.56 Moderately populated
- Cdens 0.9 Very dense
- CC3 1.0 Very high quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
CWWL 3078 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 71.694 | 60.877 | 0.233 | 0.551 | -0.102 | -18.761 |
| Hu & Soubiran | 2025 | 71.72 | 60.846 | â | â | â | â |
| Hunt & Reffert | 2024 | 71.77 | 60.859 | 0.222 | 0.587 | -0.145 | -23.444 |
| Cavallo et al. | 2024 | 71.72 | 60.846 | 0.223 | â | â | â |
| Hunt & Reffert | 2023 | 71.77 | 60.859 | 0.222 | 0.587 | -0.145 | -23.444 |
| Chi et al. | 2023 | 71.701 | 60.871 | 0.267 | 0.543 | -0.083 | 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 | 3.64 | 1.93 | 1.94 | 1175 | -0.210 | 761 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.070(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 761(1) | â | â |
| Cavallo et al. | 2024 | 3.39 | 1.92 | â | 1175 | -0.210 | â | â | â |
| Hunt & Reffert | 2023 | 3.89 | 1.94 | 1.94 | 547 | â | â | â | â |
| Chi et al. | 2023 | â | â | â | 1400 | -0.642 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.