CWNU 4756

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C3
N_50
r_50
DC 26 5.9
Summary

CWNU 4756 is a poorly populated, very loose object of very 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) 151.403 -51.264 0.127 -4.608 2.968 43.92
           
UCC 151.376 -51.248 0.113 -4.615 2.968 43.921
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4756 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.3, m-M=14.05, logA=9.5

Search coordinates in Bayestar19

Cluster region map