CWNU 4133

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C3
N_50
r_50
BB 25 5.1
Summary

CWNU 4133 is a poorly populated, very loose object of intermediate C3 quality. It is located at a 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) 278.527 -19.613 0.124 -3.226 -5.33 8.36
           
UCC 278.551 -19.612 0.132 -3.224 -5.332 -9.591
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4133 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.35, m-M=15.7, logA=9.6

Search coordinates in Bayestar19

Cluster region map