CWNU 223

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C3
N_50
r_50
BC 23 12.8
Summary

CWNU 223 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a significant percentage of members with a later reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 126.631 -33.549 0.74 -4.88 4.44
           
UCC 126.594 -33.658 0.73 -4.87 4.427 35.064
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 223 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=0.45, m-M=10.35, logAge=7.5, Z=0.012

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 5320 60.0 126.65 -33.71 0.74 -4.85 4.41 37.34 0.14