CWNU 3319

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C3
N_50
r_50
CC 47 3.1
Summary

CWNU 3319 is a poorly populated, loose object of low C3 quality. It is located at a large distance from the Sun, below 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) 89.73 15.78 0.139 0.576 -0.785 29.66
           
UCC 89.724 15.772 0.166 0.59 -0.774 29.656
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3319 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.4, m-M=13.2, logA=9.2

Search coordinates in Bayestar19

Cluster region map