CWNU 3429

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C3
N_50
r_50
DB 27 3.9
Summary

CWNU 3429 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) 158.769 -55.188 0.138 -6.23 3.03 30.22
           
UCC 158.765 -55.185 0.168 -6.25 3.026 30.22
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3429 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.9, m-M=14.05, logA=8.4

Search coordinates in Bayestar19

Cluster region map