CWNU 485

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C3
N_50
r_50
CB 31 2.2
Summary

CWNU 485 is a poorly populated, very dense 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.

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) 198.843 -61.603 0.57 -6.77 -1.69
           
UCC 198.849 -61.597 0.576 -6.772 -1.697
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 485 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=1.85, m-M=10.7, logAge=9.2, Z=0.002

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0596 96.8 198.85 -61.59 0.57 -6.77 -1.7 0.47