CWNU 4391

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.07 0.12 0.0 1.0
C3
N_50
r_50
DC 21 4.8
Summary

CWNU 4391 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It was recently reported in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

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) 29.12 54.95 0.18 -0.855 -0.233 –
           
UCC 29.133 54.954 0.177 -0.844 -0.244 -28.258
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4391 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.65, m-M=15.25, logA=7.5

Search coordinates in Bayestar19

Cluster region map