CWNU 4711

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C3
N_50
r_50
DB 20 2.6
Summary

CWNU 4711 is a sparse, very loose object of low 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: contains less than 25 stars with P>0.5 estimated.

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) 265.826 -34.364 0.039 -3.582 -5.702 -38.8
           
UCC 265.818 -34.388 0.025 -3.571 -5.738 69.836
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4711 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=3.3, m-M=16.65, logA=8.8

Search coordinates in Bayestar19

Cluster region map