CWNU 4811

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C3
N_50
r_50
BC 38 5.4
Summary

CWNU 4811 is a poorly populated, very loose object of low 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) 84.594 20.187 0.107 0.53 -0.679
           
UCC 84.622 20.171 0.112 0.464 -0.658 7.517
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4811 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.25, m-M=14.75, logA=8.0

Search coordinates in Bayestar19

Cluster region map