CWNU 4380

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C3
N_50
r_50
BC 29 2.9
Summary

CWNU 4380 is a poorly populated, very loose object of low C3 quality. It is located at a very large distance from the Sun, well 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) 165.077 -64.888 0.088 -4.435 1.888 35.43
           
UCC 165.123 -64.87 0.075 -4.483 1.84 42.185
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4380 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.6, m-M=14.6, logA=9.5

Search coordinates in Bayestar19

Cluster region map