CWNU 4106

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.28 0.18 0.25 0.0 0.82
C3
N_50
r_50
CC 28 12.5
Summary

CWNU 4106 is a poorly populated, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.82) 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) 101.702 7.535 0.667 -1.539 0.527 –
           
UCC 101.684 7.543 0.655 -1.539 0.533 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4106 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.25, m-M=10.9, logA=8.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 2118 17.9 101.74 7.37 0.64 -1.54 0.21 -4.67 0.18