CWNU 177

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C3
N_50
r_50
AB 32 11.6
Summary

CWNU 177 is a poorly populated, very loose object of high 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) 6.585 52.74 0.57 -2.0 -1.27
           
UCC 6.567 52.73 0.566 -1.995 -1.27
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 177 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=0.65, m-M=11.0, logAge=7.7, Z=0.008

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1202 100.0 6.5 52.75 0.56 -1.99 -1.27 -17.01 0.33
OC 0224 50.0 6.64 52.91 0.57 -2.04 -1.24 -7.39 0.03
Theia 2936 43.8 6.1 52.74 0.57 -1.99 -1.32 -37.72 0.01
UBC 1197 6.2 5.36 52.69 0.55 -2.02 -1.35 -37.29 0.12