CWNU 4672

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.06 0.25 0.0 1.0
C3
N_50
r_50
DB 16 5.4
Summary

CWNU 4672 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) 144.493 -51.971 0.221 -4.095 3.067 –
           
UCC 144.497 -51.993 0.221 -4.081 3.085 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4672 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=4.8, m-M=13.9, logA=7.0

Search coordinates in Bayestar19

Cluster region map