CWNU 4105

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C3
N_50
r_50
CC 15 5.1
Summary

CWNU 4105 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well above 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) 166.213 -55.865 0.124 -5.085 1.764 31.82
           
UCC 166.15 -55.853 0.122 -5.08 1.785 39.247
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4105 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.7, m-M=15.65, logA=8.0

Search coordinates in Bayestar19

Cluster region map