CWNU 1251

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C3
N_50
r_50
CB 31 65.1
Summary

CWNU 1251 is a poorly populated, very loose object of low C3 quality. It is located at a very close 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. (2022) 80.006 -6.971 3.744 -1.465 -0.107
           
UCC 79.639 -6.847 3.469 -0.242 -0.226 14.289
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1251 UCC

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.55, logAge=7.7

Search coordinates in Bayestar19

Cluster region map