CWNU 188

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C3
N_50
r_50
BB 23 7.6
Summary

CWNU 188 is a sparse, moderately dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It was recently reported in the literature.

Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 135.743 -46.724 0.87 -6.1 4.01
He et al. (2022) 135.72 -46.699 0.878 -6.1 3.997
           
UCC 135.694 -46.73 0.875 -6.109 4.007 26.501
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 188 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=2.5, m-M=10.3, logAge=7.7, Z=0.018
He et al. (2022) A0=3.15, logAge=7.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14384 100.0 135.76 -46.73 0.87 -6.11 4.01 12.22 0.26
Theia 1858 100.0 135.75 -46.73 0.87 -6.09 3.99 8.7 0.2
OC 0496 84.0 135.71 -46.74 0.87 -6.08 4.02 26.5 0.28