CWNU 4092

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C3
N_50
r_50
DC 38 2.4
Summary

CWNU 4092 is a poorly populated, moderately dense object of very low C3 quality. It is located at a moderate 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) 318.352 49.879 0.198 -2.703 -3.088
           
UCC 318.349 49.879 0.2 -2.71 -3.087
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4092 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.95, m-M=12.65, logA=7.3

Search coordinates in Bayestar19

Cluster region map