CWNU 1764

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C3
N_50
r_50
CB 24 5.8
Summary

CWNU 1764 is a sparse, moderately dense object of low C3 quality. It is located at a relatively close distance from the Sun, near 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) 152.049 -56.308 0.625 -7.735 3.946 0.19
           
UCC 152.057 -56.318 0.623 -7.735 3.967 -0.884
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1764 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.5, m-M=11.15, logAge=6.9

Search coordinates in Bayestar19

Cluster region map