CWNU 4398

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C3
N_50
r_50
DC 16 6.7
Summary

CWNU 4398 is a sparse, very loose object of very 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) 287.067 15.75 0.173 -1.913 -4.904
           
UCC 287.062 15.751 0.173 -1.925 -4.904 -71.758
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4398 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.9, m-M=13.25, logA=9.2

Search coordinates in Bayestar19

Cluster region map