CWNU 3493

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C3
N_50
r_50
BB 16 5.3
Summary

CWNU 3493 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

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) 158.434 -60.885 0.144 -4.556 2.61
           
UCC 158.412 -60.857 0.14 -4.549 2.609 29.646
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3493 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.75, m-M=14.6, logA=9.1

Search coordinates in Bayestar19

Cluster region map