CWNU 323

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C3
N_50
r_50
BB 39 24.2
Summary

CWNU 323 is a poorly populated, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a significant percentage of members with a later reported entry.

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. (2022) 124.477 -55.608 0.96 -1.24 1.53 -6.4
           
UCC 124.453 -55.642 0.957 -1.237 1.53 -3.0
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 323 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=0.8, m-M=9.65, logAge=9.2, Z=0.008

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 7593 64.1 124.32 -55.64 0.96 -1.24 1.53 -2.55 0.0