CWNU 1112

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C3
N_50
r_50
BC 21 21.9
Summary

CWNU 1112 is a sparse, very 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 significant percentage of members with a later reported entry.

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) 112.67 -14.036 0.884 -3.148 1.014
           
UCC 112.625 -14.123 0.88 -3.212 1.075 17.15
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1112 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) A0=0.55, logAge=8.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 3581 64.0 112.31 -14.19 0.89 -3.32 1.07 16.63 0.24