CWNU 4077

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C3
N_50
r_50
DB 17 1.3
Summary

CWNU 4077 is a sparse, very loose object of low C3 quality. It is located at a very 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) 267.884 -36.317 0.077 -2.457 -4.406
           
UCC 267.882 -36.317 0.054 -2.458 -4.406 106.44
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4077 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.55, m-M=15.25, logA=8.0

Search coordinates in Bayestar19

Cluster region map