CWNU 4675

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C3
N_50
r_50
DC 27 3.6
Summary

CWNU 4675 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above 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) 101.258 5.207 0.216 0.056 -0.354 84.47
           
UCC 101.269 5.253 0.201 0.067 -0.303
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4675 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.65, m-M=13.2, logA=8.9

Search coordinates in Bayestar19

Cluster region map