CWNU 3391

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C3
N_50
r_50
BC 31 3.8
Summary

CWNU 3391 is a poorly populated, loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) 110.022 -13.391 0.244 -0.635 0.747 48.73
           
UCC 110.015 -13.386 0.233 -0.654 0.742 48.734
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3391 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.3, m-M=12.95, logA=8.7

Search coordinates in Bayestar19

Cluster region map