CWNU 454
0.56
UTI
0.3
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
1.1 [arcmin]
- CN 0.3 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 454 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Distant
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 11.998 | 63.915 | 0.299 | -2.366 | -0.2 | â |
| Hunt & Reffert | 2024 | 11.995 | 63.912 | 0.296 | -2.362 | -0.2 | â |
| Cavallo et al. | 2024 | 11.967 | 63.921 | 0.295 | â | â | â |
| Hunt & Reffert | 2023 | 11.995 | 63.912 | 0.296 | -2.362 | -0.2 | â |
| He et al. | 2022 | 11.957 | 63.917 | 0.3 | -2.36 | -0.26 | 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 | 402* | â | â |
| Cavallo et al. | 2024 | 3.42 | 2.58 | â | 49 | 0.050 | â | â | â |
| Hunt & Reffert | 2023 | 3.08 | 2.57 | 0.93 | 60 | â | â | â | â |
| He et al. | 2022 | 5.01 | 3.06 | â | 6 | 0.916 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.