CWNU 2009

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C3
N_50
r_50
DC 25 3.3
Summary

CWNU 2009 is a poorly populated, loose object of very low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

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) 112.377 -21.163 0.277 -1.547 3.658
           
UCC 112.377 -21.162 0.275 -1.546 3.658
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 2009 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.75, m-M=12.5, logAge=8.2

Search coordinates in Bayestar19

Cluster region map