CWNU 3921

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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
BC 21 3.5
Summary

CWNU 3921 is a sparse, very loose object of low C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It was recently reported in the literature.

This object shares a small percentage of members with at least one entry reported in the same catalogue.

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) 108.478 -24.109 0.076 -0.538 1.53 73.05
           
UCC 108.498 -24.09 0.087 -0.527 1.542 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3921 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.3, m-M=14.75, logA=8.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3432 12.0 108.39 -24.02 0.12 -0.53 1.4 – 0.08