CWNU 345

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C3
N_50
r_50
BC 30 18.4
Summary

CWNU 345 is a poorly populated, very loose object of low C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with a later reported entry.

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. (2022) 18.928 71.177 1.02 2.33 0.33 20.7
           
UCC 18.894 71.182 1.0 2.298 0.343 9.558
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 345 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=0.95, m-M=10.4, logAge=7.9, Z=0.038

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 3502 80.0 18.9 71.23 1.0 2.31 0.36 20.14 0.01