CWNU 4600

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.25 0.21 0.12 0.0 1.0
C3
N_50
r_50
CD 25 10.2
Summary

CWNU 4600 is a poorly populated, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

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) 115.147 -12.938 0.646 -4.415 0.676 –
           
UCC 115.183 -12.915 0.609 -4.271 0.631 44.256
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4600 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.45, m-M=11.05, logA=9.4

Search coordinates in Bayestar19

Cluster region map