CWNU 3418

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C3
N_50
r_50
AB 32 3.3
Summary

CWNU 3418 is a poorly populated, very loose object of high 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) 119.218 -27.286 0.165 -1.855 2.224 84.67
           
UCC 119.215 -27.28 0.147 -1.864 2.235 84.671
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3418 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.2, m-M=14.1, logA=7.8

Search coordinates in Bayestar19

Cluster region map