CWNU 2455

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C3
N_50
r_50
AB 27 4.2
Summary

CWNU 2455 is a poorly populated, very loose object of high C3 quality. It is located at a large distance from the Sun, near 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) 115.944 -23.672 0.186 -1.331 2.062
           
UCC 115.938 -23.659 0.181 -1.34 2.038
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2455 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.7, m-M=13.55, logAge=7.8

Search coordinates in Bayestar19

Cluster region map