CWNU 4295

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C3
N_50
r_50
DB 32 2.2
Summary

CWNU 4295 is a poorly populated, very loose object of low C3 quality. It is located at a large 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) 185.786 -64.672 0.141 -6.1 0.564
           
UCC 185.783 -64.683 0.12 -6.11 0.554 42.101
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4295 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.55, m-M=13.65, logA=9.2

Search coordinates in Bayestar19

Cluster region map