CWNU 4345

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.13 0.75 0.0 0.8
C3
N_50
r_50
AB 22 8.3
Summary

CWNU 4345 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) 38.554 56.824 0.394 -0.302 -1.182 –
           
UCC 38.578 56.863 0.413 -0.301 -1.184 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4345 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.0, m-M=11.9, logA=7.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 599 20.0 38.09 56.75 0.36 -0.18 -1.21 – 0.09