CWNU 4765

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C3
N_50
r_50
BB 13 7.7
Summary

CWNU 4765 is a sparse, very loose object of intermediate 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) 271.047 -36.819 0.106 -2.872 -4.52
           
UCC 271.05 -36.829 0.133 -2.872 -4.469 -107.472
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4765 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.6, m-M=14.5, logA=9.7

Search coordinates in Bayestar19

Cluster region map