CWNU 4019

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C3
N_50
r_50
CC 22 2.4
Summary

CWNU 4019 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well 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) 231.976 -61.341 0.096 -5.506 -4.562 -20.37
           
UCC 231.975 -61.338 0.106 -5.52 -4.618 -58.495
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4019 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.65, m-M=13.65, logA=9.6

Search coordinates in Bayestar19

Cluster region map