CWNU 2614
0.21
UTI
0.0
CN
0.07
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
5.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.07 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 2614 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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.
Distant
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 | 351.61 | 64.139 | 0.208 | -2.398 | -1.022 | -26.201 |
| Hunt & Reffert | 2024 | 351.581 | 64.129 | 0.202 | -2.385 | -1.018 | -26.221 |
| Cavallo et al. | 2024 | 351.627 | 64.146 | 0.201 | â | â | â |
| Hunt & Reffert | 2023 | 351.581 | 64.129 | 0.202 | -2.385 | -1.018 | -26.221 |
| He et al. | 2023 | 351.774 | 64.191 | 0.206 | -2.398 | -1.022 | 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 | 339* | â | â |
| Cavallo et al. | 2024 | 3.94 | 2.79 | â | 54 | 0.420 | â | â | â |
| Hunt & Reffert | 2023 | 4.42 | 3.00 | 2.05 | 20 | â | â | â | â |
| He et al. | 2023 | 5.89 | 3.55 | â | 4 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.