CWNU 88
0.37
UTI
0.29
CN
0.8
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
17.0 [arcmin]
- CN 0.29 Poorly populated
- Cdens 0.8 Dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
CWNU 88 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a metal-poor, very young cluster (see Parameters). It is rarely studied in the literature.
Close
Low extinction
Metal-poor
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 131.507 | -59.87 | 1.831 | -7.836 | 6.4 | 18.577 |
| Cavallo et al. | 2024 | 131.211 | -59.244 | 1.839 | â | â | â |
| Hunt & Reffert | 2023 | 131.173 | -59.96 | 1.829 | -7.708 | 6.617 | 14.799 |
| He et al. | 2022 | 131.661 | -59.696 | 1.83 | -7.71 | 6.42 | 18.5 |
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 | 0.56 | 0.93 | â | 8 | -0.170 | â | â | â |
| Hunt & Reffert | 2023 | 0.52 | 0.28 | 0.65 | 15 | â | â | â | â |
| He et al. | 2022 | 0.48 | 0.06 | â | 8 | -0.930 | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.