CWNU 4392

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.4 0.17 0.62 0.0 1.0
C3
N_50
r_50
AC 40 5.6
Summary

CWNU 4392 is a poorly populated, very loose object of intermediate C3 quality. It is located at a moderate 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) 94.098 12.884 0.223 0.359 -0.25 60.2
           
UCC 94.107 12.875 0.236 0.413 -0.266 60.643
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 4392 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.75, m-M=13.7, logA=8.1

Search coordinates in Bayestar19

Cluster region map