CWNU 3488

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C3
N_50
r_50
AB 31 3.4
Summary

CWNU 3488 is a poorly populated, very loose object of high 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: 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) 105.893 -18.567 0.141 -0.483 1.689 84.42
           
UCC 105.887 -18.556 0.142 -0.462 1.677 84.417
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3488 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.45, m-M=14.05, logA=7.5

Search coordinates in Bayestar19

Cluster region map