CWNU 4386

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.03 0.38 0.0 1.0
C3
N_50
r_50
CB 21 2.3
Summary

CWNU 4386 is a sparse, very loose object of low C3 quality. It is located at a very large distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a significant percentage of members with a later 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=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) 294.765 26.21 0.064 -2.263 -4.39 –
           
UCC 294.766 26.205 0.059 -2.263 -4.39 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4386 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=4.0, m-M=16.0, logA=6.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 502 72.0 294.8 26.25 0.05 -2.25 -4.37 – 0.02