CWNU 4465

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C3
N_50
r_50
BB 25 2.7
Summary

CWNU 4465 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well 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) 267.543 -36.894 0.042 -2.922 -6.587 -100.9
           
UCC 267.535 -36.894 0.064 -2.908 -6.609 -75.478
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4465 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.4, m-M=17.4, logA=8.9

Search coordinates in Bayestar19

Cluster region map