CWNU 4458

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C3
N_50
r_50
CC 26 4.9
Summary

CWNU 4458 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) 287.027 11.027 0.111 -2.735 -5.753 25.94
           
UCC 287.016 11.015 0.103 -2.707 -5.756 32.652
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4458 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.9, m-M=16.4, logA=8.9

Search coordinates in Bayestar19

Cluster region map