CWNU 192

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C3
N_50
r_50
AB 24 2.7
Summary

CWNU 192 is a sparse, moderately dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.

Warning: This is very 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) 107.353 0.523 0.3 -1.02 -0.67
           
UCC 107.347 0.529 0.297 -1.016 -0.675
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 192 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=0.6, m-M=12.85, logAge=8.5, Z=0.04

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1344 100.0 107.35 0.54 0.28 -1.01 -0.68 59.45 0.5
CWWDL 12546 96.0 107.35 0.53 0.3 -1.0 -0.67 59.45 0.0
CWWDL 12541 72.0 107.35 0.53 0.28 -1.0 -0.66 0.0