CWWL 2084
0.19
UTI
0.28
CN
0.08
Cdens
0.38
CC3
0.3
Clit
0.71
Cdup
Stellar density (N50/rad)
0.4 [N/pc2]
- CN 0.28 Poorly populated
- Cdens 0.08 Very loose
- CC3 0.38 Low quality
- Clit 0.3 Poorly studied
- Cdup 0.71 Likely unique
Overview
CWWL 2084 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a metal-poor, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a small percentage with at least one entry reported in the same catalogue. 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 | 115.698 | -21.061 | 0.271 | -2.112 | 2.883 | 102.468 |
| Hunt & Reffert | 2024 | 115.684 | -21.062 | 0.281 | -2.127 | 2.948 | 102.456 |
| Cavallo et al. | 2024 | 115.753 | -21.134 | 0.282 | â | â | â |
| Hunt & Reffert | 2023 | 115.684 | -21.062 | 0.281 | -2.127 | 2.948 | 102.456 |
| Chi et al. | 2023 | 115.716 | -21.029 | 0.259 | -2.049 | 2.656 | 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 | 3.1 | 0.69 | 1.22 | 68 | -0.787 | 218 | â | â |
| Liu et al. | 2025 | 4.83 | 0.37 | â | 35 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 218(1) | â | â |
| Cavallo et al. | 2024 | 2.74 | 1.07 | â | 32 | -0.240 | â | â | â |
| Hunt & Reffert | 2023 | 3.10 | 0.69 | 1.22 | 136 | â | â | â | â |
| Chi et al. | 2023 | â | â | â | 100 | -1.335 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 120 along with HSC_1880.
Palma et al. (2025)
Part of multiple system G60, along with HSC_1880 and CWNU_2909.
Cavallo et al. (2024)
Gold sample.