CWNU 4717

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C3
N_50
r_50
CC 17 7.2
Summary

CWNU 4717 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well above 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) 327.448 59.506 0.101 -2.343 -1.609
           
UCC 327.448 59.487 0.116 -2.311 -1.606 -122.799
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4717 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.95, m-M=14.05, logA=8.9

Search coordinates in Bayestar19

Cluster region map