CWNU 95
0.23
UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.31
Clit
0.4
Cdup
Radius (P>50% members)
3.5 [arcmin]
- CN 0.47 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 0.4 Possibly duplicate
Overview
CWNU 95 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, very young cluster (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.
Relatively close
Moderate extinction
Very metal-poor
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 223.292 | -54.102 | 0.909 | -2.796 | -2.301 | -17.204 |
| Hunt & Reffert | 2024 | 223.297 | -54.112 | 0.904 | -2.858 | -2.311 | -15.491 |
| Cavallo et al. | 2024 | 222.843 | -54.217 | 0.913 | â | â | â |
| Hunt & Reffert | 2023 | 223.297 | -54.112 | 0.904 | -2.858 | -2.311 | -15.491 |
| He et al. | 2022 | 223.304 | -54.118 | 0.901 | -2.806 | -2.3 | â |
| He et al. | 2022 | 223.296 | -54.111 | 0.91 | -2.8 | -2.3 | 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 | 184* | â | â |
| Cavallo et al. | 2024 | 1.08 | 1.15 | â | 12 | -0.050 | â | â | â |
| Hunt & Reffert | 2023 | 1.03 | 1.08 | 1.41 | 23 | â | â | â | â |
| He et al. | 2022 | â | 1.05 | â | 11 | â | â | â | â |
| He et al. | 2022 | 0.85 | 1.38 | â | 16 | -2.028 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.