CWNU 2367
0.18
UTI
0.0
CN
0.16
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
8.5 [arcmin]
- CN 0.0 Sparse
- Cdens 0.16 Very loose
- CC3 0.25 Low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 2367 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (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.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 341.03 | 57.6 | 0.487 | -3.324 | -1.483 | -45.259 |
| Hunt & Reffert | 2024 | 341.115 | 57.607 | 0.486 | -3.311 | -1.516 | -45.238 |
| Cavallo et al. | 2024 | 341.071 | 57.59 | 0.484 | â | â | â |
| Hunt & Reffert | 2023 | 341.115 | 57.607 | 0.486 | -3.311 | -1.516 | -45.238 |
| He et al. | 2023 | 341.062 | 57.603 | 0.491 | -3.32 | -1.499 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 150* | â | â |
| Cavallo et al. | 2024 | 2.25 | 1.53 | â | 34 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 1.99 | 1.42 | 0.41 | 52 | â | â | â | â |
| He et al. | 2023 | 1.95 | 1.45 | â | 56 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.