CWNU 4108

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.06 0.75 0.0 0.8
C3
N_50
r_50
AB 18 9.7
Summary

CWNU 4108 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.

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

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.8) 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) 26.86 60.433 0.356 -1.04 -0.562 –
           
UCC 26.729 60.439 0.361 -1.044 -0.58 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4108 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.9, m-M=12.05, logA=7.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1332 20.0 26.93 60.44 0.34 -1.02 -0.47 – 0.19