CWNU 54

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C3
N_50
r_50
DC 16 34.4
Summary

CWNU 54 is a sparse, very loose object of very low C3 quality. It is located at a close 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. (2022) 120.406 -54.297 1.34 -3.3 6.26 16.9
           
UCC 120.639 -54.28 1.333 -3.237 6.267 25.56
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 54 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=0.5, m-M=9.5, logAge=8.9, Z=0.02

Search coordinates in Bayestar19

Cluster region map