CWNU 483

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0.05 UTI
0.5
CN
0.23
Cdens
0.38
CC3
0.0
Clit
0.24
Cdup
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

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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.

âš 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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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 –
He et al. 2022 51.096 54.875 0.43 0.39 -1.06 -26.7

💡 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 99999– 3.635 3.395 – 710 0.259 – – 1
Li et al. 2023 3.80 2.35 – 1413 0.097 – – 1(1)
He et al. 2022 3.47 4.44 – 6 0.420 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0266 76.0 51.17 54.9 0.43 0.29 -1.02 19.57 0.29

💡 Note: The % column shows the percentage of members that CWNU 483 shares with each listed object.

Visualization

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