CWNU 190

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C3
N_50
r_50
CB 25 2.7
Summary

CWNU 190 is a poorly populated, very dense object of low C3 quality. It is located at a relatively close distance from the Sun, below 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 105.181 -14.395 0.63 -1.39 1.65 28.1
           
UCC 105.175 -14.383 0.624 -1.403 1.637 21.55
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 190 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=1.0, m-M=10.95, logAge=9.0, Z=0.012

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0381 96.0 105.17 -14.39 0.63 -1.41 1.64 21.55 0.49