CWNU 4096

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.02 0.25 0.0 1.0
C3
N_50
r_50
CC 13 4.7
Summary

CWNU 4096 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It was recently reported in the literature.

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) 138.212 -58.087 0.119 -2.994 3.244 83.95
           
UCC 138.214 -58.079 0.12 -3.011 3.275 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4096 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.6, m-M=14.3, logA=9.6

Search coordinates in Bayestar19

Cluster region map