CWNU 1106
0.40
UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
9.6 [arcmin]
- CN 0.0 Sparse
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
CWNU 1106 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is rarely studied in the literature.
Very 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 | 87.587 | 8.207 | 2.443 | -3.486 | -3.653 | 24.937 |
| Cavallo et al. | 2024 | 87.667 | 8.204 | 2.455 | â | â | â |
| Hunt & Reffert | 2023 | 87.587 | 8.231 | 2.442 | -3.432 | -3.638 | 46.874 |
| He et al. | 2022 | 87.591 | 8.176 | 2.478 | -3.5 | -3.645 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.46 | 1.43 | â | 59 | 0.420 | â | â | â |
| Hunt & Reffert | 2023 | 0.38 | 0.46 | 0.66 | 4 | â | â | â | â |
| He et al. | 2022 | â | 0.05 | â | 3 | â | â | â | â |
Cavallo et al. (2024)
Wood sample.
Hunt & Reffert (2024)
Classified as a moving group.