CWNU 3593

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C3
N_50
r_50
AC 57 4.0
Summary

CWNU 3593 is a moderately 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.

This object shares a very small percentage of members with at least one entry reported in the same catalogue.

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) 167.948 -67.89 0.095 -5.2 1.978 21.58
           
UCC 167.909 -67.891 0.082 -5.167 1.974 6.513
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3593 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.6, m-M=14.05, logA=9.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4856 1.8 168.23 -67.75 0.23 -5.52 1.77 -21.62 0.04