CWNU 483
0.05
UTI
0.5
CN
0.23
Cdens
0.38
CC3
0.0
Clit
0.24
Cdup
Nm (P>50%)
50
Core radius and density
1.8 [pc], 1.1 [pc-2]
- CN 0.5 Moderately populated
- Cdens 0.23 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.24 Likely duplicate
Overview
CWNU 483 is a moderately populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is rarely studied in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
(*): The parallax distance estimate (~2.32 kpc) differs significantly from the median photometric distance (~3.63 kpc).
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 51.135 | 54.87 | 0.43 | 0.359 | -1.084 | -26.589 |
| Li et al. | 2023 | 51.162 | 54.912 | 0.41 | 0.33 | -1.03 | â |
| He et al. | 2022 | 51.096 | 54.875 | 0.43 | 0.39 | -1.06 | -26.7 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.635 | 3.395 | â | 710 | 0.259 | â | â | 1 |
| Li et al. | 2023 | 3.80 | 2.35 | â | 1413 | 0.097 | â | â | 1(1) |
| He et al. | 2022 | 3.47 | 4.44 | â | 6 | 0.420 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
