CWNU 4488

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C3
N_50
r_50
CB 27 5.7
Summary

CWNU 4488 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below 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. (2023) 260.24 -46.89 0.204 -2.443 -4.629
           
UCC 260.267 -46.89 0.204 -2.438 -4.662 -39.677
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4488 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.6, m-M=13.5, logA=9.4

Search coordinates in Bayestar19

Cluster region map