CWNU 4395

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.25 0.66 0.25 0.0 1.0
C3
N_50
r_50
DB 25 1.6
Summary

CWNU 4395 is a poorly populated, moderately dense 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 small percentage of members with a later reported entry.

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) 330.028 59.476 0.165 -2.529 -1.91 –
           
UCC 330.012 59.469 0.169 -2.552 -1.913 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4395 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.3, m-M=14.85, logA=6.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 4560 20.0 330.01 59.47 0.15 -2.38 -1.85 – 0.04