CWNU 348
0.46
UTI
0.49
CN
1.0
Cdens
0.62
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
49
Core radius and density
0.8 [pc], 9.7 [pc-2]
- CN 0.49 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.1 Rarely studied
- Cdup 1.0 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 348 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is rarely studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 328.11 | 64.939 | 0.897 | -2.124 | -4.561 | -27.998 |
| Hunt & Reffert | 2024 | 328.135 | 64.946 | 0.917 | -2.097 | -4.572 | -11.014 |
| Cavallo et al. | 2024 | 328.119 | 64.966 | 0.902 | â | â | â |
| Hunt & Reffert | 2023 | 328.135 | 64.946 | 0.917 | -2.097 | -4.572 | -11.014 |
| He et al. | 2022 | 328.117 | 64.96 | 0.889 | -2.135 | -4.579 | â |
| He et al. | 2022 | 328.125 | 64.967 | 0.89 | -2.13 | -4.56 | -10.6 |
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 | 1.1 | 1.35 | 2.31 | 6 | 0.045 | 89 | â | â |
| Hunt & Reffert | 2024 | 1.10 | 1.46 | 2.31 | 6 | â | 89(1) | â | â |
| Cavallo et al. | 2024 | 1.15 | 1.27 | â | 48 | 0.370 | â | â | â |
| Hunt & Reffert | 2023 | 1.10 | 1.46 | 2.31 | 6 | â | â | â | â |
| He et al. | 2022 | â | 1.35 | â | 2 | â | â | â | â |
| He et al. | 2022 | 0.83 | 1.14 | â | 4 | -0.279 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Palma et al. (2025)
Classified as optical pair P370, along with Theia_5356.
Cavallo et al. (2024)
Wood sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.56 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.56 (50th percentile).