CWNU 4404

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C3
N_50
r_50
AB 17 3.5
Summary

CWNU 4404 is a sparse, very loose object of high C3 quality. It is located at a very 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) 219.713 -58.612 0.111 -5.276 -2.559 39.47
           
UCC 219.706 -58.618 0.093 -5.27 -2.598 21.334
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4404 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=5.0, m-M=16.3, logA=8.5

Search coordinates in Bayestar19

Cluster region map