CWNU 1168

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C3
N_50
r_50
CB 20 34.1
Summary

CWNU 1168 is a sparse, very loose object of low C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry, and a small percentage 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=0.92) 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) 277.326 4.52 2.298 0.587 -5.253
           
UCC 277.749 4.901 2.299 0.77 -5.333 -25.722
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1168 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) A0=1.2, logAge=7.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1061 12.0 276.69 3.13 2.38 1.12 -4.82 -24.41 0.15
Melotte 210 8.0 279.66 5.45 2.11 1.26 -4.95 -24.82 1.0