CWNU 3896

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C3
N_50
r_50
CC 49 1.3
Summary

CWNU 3896 is a poorly populated, loose object of low C3 quality. It is located at a very large distance from the Sun, 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) 145.16 -53.687 0.086 -4.536 3.723 93.27
           
UCC 145.16 -53.687 0.081 -4.537 3.71 93.274
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3896 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=5.1, m-M=15.8, logA=7.2

Search coordinates in Bayestar19

Cluster region map