CWNU 420

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C3
N_50
r_50
AA 40 6.4
Summary

CWNU 420 is a poorly populated, dense object of very high 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 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) 205.339 -56.681 0.58 -4.46 -1.29 -14.9
           
UCC 205.325 -56.673 0.584 -4.456 -1.284 -15.541
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 420 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=0.3, m-M=10.75, logAge=8.9, Z=0.038

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0602 82.5 205.32 -56.67 0.58 -4.46 -1.28 -15.57 0.53
CWWDL 14077 72.5 205.3 -56.67 0.58 -4.46 -1.28 -15.54 0.0