CWNU 4029

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C3
N_50
r_50
CC 20 5.1
Summary

CWNU 4029 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, 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) 126.208 -35.732 0.161 -2.509 2.932 90.84
           
UCC 126.218 -35.747 0.147 -2.505 2.902 90.842
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4029 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.2, m-M=13.0, logA=8.8

Search coordinates in Bayestar19

Cluster region map