CWNU 4768

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C3
N_50
r_50
CB 11 6.0
Summary

CWNU 4768 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well 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) 262.956 -48.903 0.108 -2.461 -4.177
           
UCC 262.9 -48.898 0.11 -2.382 -4.138 -53.099
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4768 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.25, m-M=14.05, logA=9.2

Search coordinates in Bayestar19

Cluster region map