CWNU 391

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.05 0.75 0.0 1.0
C3
N_50
r_50
AB 23 10.2
Summary

CWNU 391 is a sparse, very loose object of high C3 quality. It is located at a moderate distance from the Sun, 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. (2022) 27.273 57.558 0.32 -0.84 -0.7 –
           
UCC 27.305 57.625 0.314 -0.851 -0.692 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 391 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=0.65, m-M=12.15, logAge=8.6, Z=0.018

Search coordinates in Bayestar19

Cluster region map