CWNU 1752
0.33
UTI
0.0
CN
0.51
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
3.9 [arcmin]
- CN 0.0 Sparse
- Cdens 0.51 Moderately dense
- CC3 0.5 Intermediate quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1752 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close
Moderate 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 | 245.303 | -52.649 | 0.407 | -1.725 | -2.366 | -60.669 |
| Hu & Soubiran | 2025 | 245.303 | -52.653 | â | â | â | â |
| Hunt & Reffert | 2024 | 245.356 | -52.673 | 0.412 | -1.785 | -2.385 | -61.455 |
| Cavallo et al. | 2024 | 245.303 | -52.653 | 0.412 | â | â | â |
| Hunt & Reffert | 2023 | 245.356 | -52.673 | 0.412 | -1.785 | -2.385 | -61.455 |
| He et al. | 2023 | 245.279 | -52.638 | 0.41 | -1.72 | -2.352 | -61.46 |
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 | -0.190* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 178* | â | â |
| Cavallo et al. | 2024 | 1.81 | 1.57 | â | 537 | -0.490 | â | â | â |
| Hunt & Reffert | 2023 | 2.20 | 1.02 | 0.81 | 326 | â | â | â | â |
| He et al. | 2023 | 2.24 | 1.20 | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.