CWNU 4352

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.01 0.25 0.0 1.0
C3
N_50
r_50
DB 11 7.1
Summary

CWNU 4352 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a very small percentage of members with at least one entry reported in the same catalogue.

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) 232.09 -51.126 0.193 -4.59 -3.213 –
           
UCC 232.149 -51.126 0.156 -4.654 -3.242 -19.459
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4352 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.95, m-M=13.85, logA=9.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4358 8.0 232.3 -51.12 0.17 -4.84 -3.49 -68.06 0.16