CWNU 289

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C3
N_50
r_50
BC 35 11.4
Summary

CWNU 289 is a poorly populated, loose object of low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

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. (2022) 100.627 7.565 0.72 -1.57 0.01
He et al. (2022) 154.79 -55.861 2.266 -14.409 2.718
           
UCC 100.635 7.595 0.715 -1.617 -0.047 51.555
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 289 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=0.5, m-M=11.65, logAge=6.6, Z=0.004
He et al. (2022) A0=0.3, logAge=7.55

Search coordinates in Bayestar19

Cluster region map