CWNU 103

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C3
N_50
r_50
CC 24 12.4
Summary

CWNU 103 is a sparse, loose object of low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a moderate percentage of members with at least one entry reported in the same catalogue.

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. (2022) 30.775 68.449 0.98 0.78 0.58
           
UCC 30.683 68.445 0.984 0.754 0.574 -18.336
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 103 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=1.4, m-M=10.8, logAge=6.2, Z=0.002

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 4940 52.0 30.07 68.61 0.99 0.74 0.59 -23.86 0.09
CWNU 377 36.0 29.99 68.64 0.99 0.65 0.62 -34.08 0.15