CWNU 3965

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C3
N_50
r_50
BB 25 3.0
Summary

CWNU 3965 is a poorly populated, very 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) 121.614 -23.731 0.183 -2.259 2.377 68.45
           
UCC 121.613 -23.728 0.183 -2.262 2.377 68.454
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3965 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.55, m-M=13.4, logA=8.9

Search coordinates in Bayestar19

Cluster region map