CWNU 4275

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C3
N_50
r_50
CC 40 5.3
Summary

CWNU 4275 is a poorly populated, very loose object of low C3 quality. It is located at a large 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) 355.295 59.614 0.188 -2.181 -1.158
           
UCC 355.303 59.617 0.194 -2.134 -1.168 -97.677
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4275 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.15, m-M=13.0, logA=8.6

Search coordinates in Bayestar19

Cluster region map