CWNU 126

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C3
N_50
r_50
CB 27 6.2
Summary

CWNU 126 is a poorly populated, loose 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.

This object shares a large 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) 85.47 30.265 0.53 0.47 -2.48
           
UCC 85.482 30.278 0.536 0.47 -2.485
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 126 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=1.9, m-M=11.3, logAge=7.4, Z=0.018

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1798 100.0 85.47 30.28 0.53 0.47 -2.48 -41.97 0.08