CWNU 2032

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C3
N_50
r_50
DC 20 7.7
Summary

CWNU 2032 is a sparse, very loose object of very 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) 54.864 50.459 0.352 0.784 -1.712
           
UCC 54.836 50.461 0.342 0.784 -1.733
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2032 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.7, m-M=11.95, logAge=8.35

Search coordinates in Bayestar19

Cluster region map