CWNU 4419

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C3
N_50
r_50
DB 17 4.1
Summary

CWNU 4419 is a sparse, very loose object of low C3 quality. It is located at a large 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) 276.587 -22.534 0.194 -1.301 -6.798 116.48
           
UCC 276.582 -22.534 0.167 -1.355 -6.838 116.481
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4419 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.85, m-M=12.8, logA=9.6

Search coordinates in Bayestar19

Cluster region map