CWNU 3975

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C3
N_50
r_50
BB 26 2.1
Summary

CWNU 3975 is a poorly populated, loose object of intermediate C3 quality. It is located at a large distance from the Sun, above 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) 166.09 -58.772 0.124 -6.831 2.598 56.07
           
UCC 166.087 -58.774 0.14 -6.828 2.59 28.184
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3975 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.1, m-M=14.65, logA=9.2

Search coordinates in Bayestar19

Cluster region map