CWNU 1689

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C3
N_50
r_50
CB 15 11.2
Summary

CWNU 1689 is a sparse, very loose object of 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: 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) 194.529 -60.301 0.356 -6.93 -0.297 -26.88
           
UCC 194.632 -60.308 0.346 -6.916 -0.302 -44.423
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1689 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.4, m-M=12.1, logAge=8.5

Search coordinates in Bayestar19

Cluster region map