CWNU 4322

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C3
N_50
r_50
AB 28 5.0
Summary

CWNU 4322 is a poorly populated, very loose object of high 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) 247.932 -52.568 0.122 -4.578 -4.865 -122.21
           
UCC 247.912 -52.572 0.111 -4.56 -4.891 -75.937
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4322 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.35, m-M=15.55, logA=9.2

Search coordinates in Bayestar19

Cluster region map