CWWL 2073
0.22
UTI
0.0
CN
0.1
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
4.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.1 Very loose
- CC3 0.38 Low quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
CWWL 2073 is a sparse, 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 near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
(*): The parallax distance estimate (~4.80 kpc) differs significantly from the median photometric distance (~3.60 kpc).
Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
Distant
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 116.952 | -24.702 | 0.208 | -1.531 | 1.84 | 70.755 |
| Hu & Soubiran | 2025 | 116.988 | -24.73 | â | â | â | â |
| Hunt & Reffert | 2024 | 116.942 | -24.705 | 0.205 | -1.554 | 1.817 | 72.326 |
| Cavallo et al. | 2024 | 116.988 | -24.73 | 0.206 | â | â | â |
| Hunt & Reffert | 2023 | 116.942 | -24.705 | 0.205 | -1.554 | 1.817 | 72.326 |
| Chi et al. | 2023 | 116.97 | -24.682 | 0.23 | -1.512 | 2.117 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.170* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 157* | â | â |
| Cavallo et al. | 2024 | 3.09 | 1.14 | â | 550 | -0.230 | â | â | â |
| Hunt & Reffert | 2023 | 4.12 | 0.56 | 0.69 | 558 | â | â | â | â |
| Chi et al. | 2023 | â | â | â | 600 | 0.274 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.