CWNU 452

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.08 0.25 0.0 1.0
C3
N_50
r_50
CC 20 16.7
Summary

CWNU 452 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, well 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) 137.83 -18.544 0.8 -5.75 0.55 10.9
           
UCC 137.736 -18.657 0.682 -5.743 0.608 17.861
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 452 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=0.4, m-M=10.4, logAge=9.1, Z=0.012

Search coordinates in Bayestar19

Cluster region map