CWNU 3579

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C3
N_50
r_50
AC 32 1.9
Summary

CWNU 3579 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well 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) 111.68 -27.36 0.097 -1.011 1.738 149.33
           
UCC 111.685 -27.349 0.065 -0.999 1.688 149.327
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3579 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.4, m-M=14.9, logA=8.8

Search coordinates in Bayestar19

Cluster region map