CWNU 2024
0.19
UTI
0.0
CN
0.22
Cdens
0.62
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
23
Core radius and density
1.9 [pc], 1.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.22 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.06 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 2024 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported 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 | 287.843 | 10.521 | 0.317 | -0.526 | -3.053 | 26.065 |
| Hunt & Reffert | 2024 | 287.844 | 10.525 | 0.318 | -0.512 | -3.051 | 26.072 |
| Cavallo et al. | 2024 | 287.844 | 10.534 | 0.319 | â | â | â |
| Hunt & Reffert | 2023 | 287.844 | 10.525 | 0.318 | -0.512 | -3.051 | 26.072 |
| He et al. | 2023 | 287.844 | 10.531 | 0.34 | -0.512 | -3.045 | 26.07 |
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 | 2.81 | 4.34 | 0.31 | 312 | -0.050 | 445 | â | â |
| Hunt & Reffert | 2024 | 2.81 | 4.34 | 0.31 | 312 | â | 445(1) | â | â |
| Cavallo et al. | 2024 | 3.34 | 4.52 | â | 224 | -0.050 | â | â | â |
| Hunt & Reffert | 2023 | 2.81 | 4.34 | 0.31 | 312 | â | â | â | â |
| He et al. | 2023 | 2.63 | 4.15 | â | 891 | 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.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 1.00 (50th percentile), true positive? (human-assigned).
Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 1.00 (50th percentile), true positive? (human-assigned).