CWNU 396

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.57 0.12 0.0 1.0
C3
N_50
r_50
DC 22 11.0
Summary

CWNU 396 is a sparse, moderately dense object of very low C3 quality. It is located at a close distance from the Sun, above 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) 80.811 64.656 1.18 2.55 -4.88 3.1
           
UCC 80.769 64.702 1.153 2.591 -4.937 5.361
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 396 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=1.7, m-M=10.55, logAge=7.3, Z=0.004

Search coordinates in Bayestar19

Cluster region map