CWNU 334
0.19
UTI
0.28
CN
0.21
Cdens
0.25
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
28
Core radius and density
1.2 [pc], 1.0 [pc-2]
- CN 0.28 Poorly populated
- Cdens 0.21 Very loose
- CC3 0.25 Low 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 334 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is rarely studied in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 89.38 | 19.116 | 0.88 | -0.213 | -3.113 | 20.447 |
| Zhang et al. | 2024 | 89.402 | 19.265 | â | â | â | â |
| Hunt & Reffert | 2024 | 89.402 | 19.265 | 0.869 | -0.217 | -3.125 | 5.479 |
| Cavallo et al. | 2024 | 89.393 | 19.18 | 0.87 | â | â | â |
| Hunt & Reffert | 2023 | 89.402 | 19.265 | 0.869 | -0.217 | -3.125 | 5.479 |
| He et al. | 2022 | 89.45 | 19.05 | 0.9 | -0.24 | -3.02 | 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 | 1.14 | 0.9 | 1.21 | 84 | 0.280 | 134 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.136(1) | â | â | â |
| Hunt & Reffert | 2024 | 1.07 | 0.82 | 1.21 | 106 | â | 134(1) | â | â |
| Cavallo et al. | 2024 | 1.21 | 0.98 | â | 42 | 0.280 | â | â | â |
| Hunt & Reffert | 2023 | 1.07 | 0.82 | 1.21 | 106 | â | â | â | â |
| He et al. | 2022 | 1.23 | 1.01 | â | 63 | 0.398 | 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.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).