CWNU 4588

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.25 0.13 0.25 0.0 1.0
C3
N_50
r_50
CC 25 3.6
Summary

CWNU 4588 is a poorly populated, very loose object of low C3 quality. It is located at a large 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) 317.257 55.002 0.175 -2.751 -3.079 -102.12
           
UCC 317.253 54.996 0.171 -2.749 -3.079 -82.903
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 4588 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.15, m-M=13.45, logA=9.1

Search coordinates in Bayestar19

Cluster region map