CWNU 4072

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C3
N_50
r_50
BC 12 7.2
Summary

CWNU 4072 is a sparse, 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: contains less than 25 stars with P>0.5 estimated.

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) 163.313 -62.618 0.147 -4.881 2.114 26.15
           
UCC 163.286 -62.604 0.133 -4.877 2.122 26.154
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4072 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.2, m-M=14.5, logA=9.0

Search coordinates in Bayestar19

Cluster region map