CWNU 4789

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.03 0.5 0.0 1.0
C3
N_50
r_50
BB 16 4.0
Summary

CWNU 4789 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, above 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) 173.657 -60.812 0.101 -6.257 1.563 –
           
UCC 173.688 -60.832 0.11 -6.245 1.558 5.047
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4789 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.55, m-M=13.85, logA=6.8

Search coordinates in Bayestar19

Cluster region map