CWNU 2170

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C3
N_50
r_50
DC 18 10.0
Summary

CWNU 2170 is a sparse, very loose object of very 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: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 133.83 -40.882 0.7 -3.912 3.642 34.43
           
UCC 133.916 -40.903 0.691 -3.919 3.615 15.034
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2170 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.85, m-M=10.6, logAge=8.85

Search coordinates in Bayestar19

Cluster region map