CWNU 4152

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C3
N_50
r_50
DB 28 3.9
Summary

CWNU 4152 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) 324.283 55.397 0.125 -2.438 -2.245
           
UCC 324.25 55.393 0.12 -2.431 -2.225
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4152 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.75, m-M=15.45, logA=6.7

Search coordinates in Bayestar19

Cluster region map