CWNU 4218

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C3
N_50
r_50
AB 27 3.5
Summary

CWNU 4218 is a poorly populated, very loose object of high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

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. (2023) 115.08 -30.152 0.111 -1.035 2.13
           
UCC 115.094 -30.157 0.112 -1.027 2.105 101.359
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4218 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.5, m-M=14.65, logA=8.8

Search coordinates in Bayestar19

Cluster region map