CWNU 2352
0.54
UTI
0.31
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.97
Cdup
Stellar density (N50/rad)
6.8 [N/pc2]
- CN 0.31 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 0.97 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
CWNU 2352 is a poorly populated, very dense object of very high 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.
Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. 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 | 35.375 | 57.994 | 0.287 | -1.339 | -0.418 | â |
| Hunt & Reffert | 2024 | 35.389 | 57.998 | 0.287 | -1.337 | -0.414 | â |
| Cavallo et al. | 2024 | 35.353 | 57.997 | 0.287 | â | â | â |
| Hunt & Reffert | 2023 | 35.389 | 57.998 | 0.287 | -1.337 | -0.414 | â |
| He et al. | 2023 | 35.346 | 58.011 | 0.296 | -1.335 | -0.39 | -53.69 |
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 | 3.13 | 2.35 | 0.67 | 100 | 0.040 | 321 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 321(1) | â | â |
| Cavallo et al. | 2024 | 3.58 | 2.43 | â | 66 | 0.040 | â | â | â |
| Hunt & Reffert | 2023 | 3.13 | 2.18 | 0.67 | 100 | â | â | â | â |
| He et al. | 2023 | 3.09 | 2.35 | â | 141 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Gold sample.