CWNU 1096
0.33
UTI
0.0
CN
0.67
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
25.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.67 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
CWNU 1096 is a sparse, moderately 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 (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 | 127.547 | -38.968 | 2.738 | -6.659 | 9.632 | 3.405 |
| Cavallo et al. | 2024 | 127.549 | -39.04 | 2.733 | â | â | â |
| Hunt & Reffert | 2023 | 127.256 | -38.825 | 2.728 | -6.676 | 9.613 | -5.122 |
| He et al. | 2022 | 127.569 | -38.807 | 2.726 | -6.634 | 9.553 | 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 | 0.37 | 0.58 | â | 6 | 0.340 | â | â | â |
| Hunt & Reffert | 2023 | 0.35 | 0.53 | 0.70 | 5 | â | â | â | â |
| He et al. | 2022 | â | 0.40 | â | 8 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.