CWNU 4167

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C3
N_50
r_50
CC 33 5.1
Summary

CWNU 4167 is a poorly populated, very loose object of low 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) 311.304 36.203 0.121 -2.47 -3.678 -86.7
           
UCC 311.287 36.187 0.13 -2.498 -3.674 -79.726
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4167 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.85, m-M=14.45, logA=9.2

Search coordinates in Bayestar19

Cluster region map