CWNU 3445

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C3
N_50
r_50
DC 26 2.1
Summary

CWNU 3445 is a poorly populated, 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) 26.013 65.133 0.116 -1.035 0.523 -88.95
           
UCC 26.007 65.141 0.135 -1.044 0.529 -94.966
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3445 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.95, m-M=14.2, logA=8.9

Search coordinates in Bayestar19

Cluster region map