CWNU 4707

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C3
N_50
r_50
BC 24 4.2
Summary

CWNU 4707 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, 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) 325.345 58.924 0.162 -2.517 -2.403 -103.11
           
UCC 325.343 58.924 0.187 -2.543 -2.384 -86.585
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4707 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.75, m-M=13.4, logA=8.7

Search coordinates in Bayestar19

Cluster region map