CWNU 4185

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C3
N_50
r_50
CC 39 5.8
Summary

CWNU 4185 is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, above 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) 165.784 -56.085 0.17 -6.038 2.434 4.41
           
UCC 165.801 -56.095 0.14 -6.033 2.399 16.886
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4185 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.05, m-M=13.7, logA=9.7

Search coordinates in Bayestar19

Cluster region map