CWNU 1452

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C3
N_50
r_50
BC 26 3.1
Summary

CWNU 1452 is a poorly populated, moderately dense object of low C3 quality. It is located at a moderate distance from the Sun, above 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) 2.347 63.329 0.311 -1.923 -0.633
           
UCC 2.349 63.338 0.302 -1.931 -0.616
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1452 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.55, m-M=12.3, logAge=8.3

Search coordinates in Bayestar19

Cluster region map