CWNU 35
0.18
UTI
0.27
CN
0.25
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
26.4 [arcmin]
- CN 0.27 Poorly populated
- Cdens 0.25 Loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
CWNU 35 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (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.
Close
Low extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 92.956 | -16.553 | 1.648 | -1.633 | 1.705 | 23.046 |
| Cavallo et al. | 2024 | 92.898 | -16.515 | 1.659 | â | â | â |
| Hunt & Reffert | 2023 | 92.969 | -16.525 | 1.666 | -1.587 | 1.699 | 21.428 |
| He et al. | 2022 | 92.919 | -16.539 | 1.65 | -1.54 | 1.74 | 9.8 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.65 | 0.71 | â | 7 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 0.59 | 0.21 | 0.43 | 15 | â | â | â | â |
| He et al. | 2022 | 0.52 | 0.06 | â | 50 | 0.611 | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.