CWNU 1731

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C3
N_50
r_50
CC 22 4.7
Summary

CWNU 1731 is a sparse, loose object of low C3 quality. It is located at a moderate distance from the Sun, 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) 47.682 53.808 0.398 0.61 -1.296
           
UCC 47.647 53.822 0.347 0.567 -1.33
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1731 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.65, m-M=12.45, logAge=6.2

Search coordinates in Bayestar19

Cluster region map